Relevant bibliographies by topics / Cosmic Explosions

Academic literature on the topic 'Cosmic Explosions'

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Published: 10 December 2022
Last updated: 28 January 2023

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Journal articles on the topic "Cosmic Explosions"

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Hjorth, Jens, Chryssa Kouveliotou, and Stan Woosley. "Hunting cosmic explosions." Physics World 17, no. 10 (October 2004): 35–39. http://dx.doi.org/10.1088/2058-7058/17/10/31.

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Kulkarni, S. R. "Cosmic Explosions (Optical)." Proceedings of the International Astronomical Union 7, S285 (September 2011): 55–61. http://dx.doi.org/10.1017/s174392131200021x.

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One of the principal motivations of wide-field and synoptic surveys is the search for, and study of, transients. By transients I mean those sources that arise from the background, are detectable for some time, and then fade away to oblivion. Transients in distant galaxies need to be sufficiently bright as to be detectable, and in almost all cases those transients are catastrophic events, marking the deaths of stars. Exemplars include supernovæ and gamma-ray bursts. In our own Galaxy, the transients are strongly variable stars, and in almost all cases are at best cataclysmic rather than catastrophic. Exemplars include flares from M dwarfs, novæ of all sorts (dwarf novæ, recurrent novæ, classical novæ, X-ray novæ) and instabilities in the surface layers of stars such as S Dor or η Carina. In the nearby Universe (say out to the Virgo cluster) we have sufficient sensitivity to see novæ. In 1 I review the history of transients (which is intimately related to the advent of wide-field telescopic imaging). In 2 I summarize wide-field imaging projects, and I then review the motivations that led to the design of the Palomar Transient Factory (PTF). Next comes a summary of the astronomical returns from PTF (3), and that is followed by lessons that I have learnt from PTF (4). I conclude that, during this decade, the study of optical transients will continue to flourish (and may even accelerate as surveys at other wavelengths—notably radio, UV and X-ray—come on-line). Furthermore, it is highly likely that there will be a proliferation of highly-specialized searches for transients. Those searches may well remain active even in the era of LSST (5). I end the article by discussing the importance of follow-up telescopes for transient object studies—a topical issue, given the Portfolio Review that is being undertaken in the US.
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Hamuy, Mario. "Cosmic explosions under scrutiny." Nature 480, no. 7377 (December 2011): 328–29. http://dx.doi.org/10.1038/480328a.

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Maslyuh, V. O., and B. I. Hnatyk. "Cosmic rays from hypernovae explosions." Astronomical School’s Report 7, no. 2 (2011): 258–61. http://dx.doi.org/10.18372/2411-6602.07.2258.

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Catanzaro, Michele. "Telescope hunts for cosmic explosions." Physics World 22, no. 05 (May 2009): 7. http://dx.doi.org/10.1088/2058-7058/22/05/10.

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Biermann, Peter L., Philipp P. Kronberg, Michael L. Allen, Athina Meli, and Eun-Suk Seo. "The Origin of the Most Energetic Galactic Cosmic Rays: Supernova Explosions into Massive Star Plasma Winds." Galaxies 7, no. 2 (April 14, 2019): 48. http://dx.doi.org/10.3390/galaxies7020048.

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We propose that the high energy Cosmic Ray particles up to the upturn commonly called the ankle, from around the spectral turn-down commonly called the knee, mostly come from Blue Supergiant star explosions. At the upturn, i.e., the ankle, Cosmic Rays probably switch to another source class, most likely extragalactic sources. To show this we recently compiled a set of Radio Supernova data where we compute the magnetic field, shock speed and shock radius. This list included both Blue and Red Supergiant star explosions; both data show the same magnetic field strength for these two classes of stars despite very different wind densities and velocities. Using particle acceleration theory at shocks, those numbers can be transformed into characteristic ankle and knee energies. Without adjusting any free parameters both of these observed energies are directly indicated by the supernova data. In the next step in the argument, we use the Supernova Remnant data of the starburst galaxy M82. We apply this analysis to Blue Supergiant star explosions: The shock will race to their outer edge with a magnetic field that is observed to follow over several orders of magnitude B ( r ) × r ∼ c o n s t . , with in fact the same magnetic field strength for such stellar explosions in our Galaxy, and other galaxies including M82. The speed is observed to be ∼0.1 c out to about 10 16 cm radius in the plasma wind. The Supernova shock can run through the entire magnetic plasma wind region at full speed all the way out to the wind-shell, which is of order parsec scale in M82. We compare and identify the Cosmic Ray spectrum in other galaxies, in the starburst galaxy M82 and in our Galaxy with each other; we suggest how Blue Supergiant star explosions can provide the Cosmic Ray particles across the knee and up to the ankle energy range. The data from the ISS-CREAM (Cosmic Ray Energetics and Mass Experiment at the International Space Station) mission will test this cosmic ray concept which is reasonably well grounded in two independent radio supernova data sets. The next step in developing our understanding will be to obtain future more accurate Cosmic Ray data near to the knee, and to use unstable isotopes of Cosmic Ray nuclei at high energy to probe the “piston” driving the explosion. We plan to incorporate these data with the physics of the budding black hole which is probably forming in each of these stars.
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de Souza, R. S., E. E. O. Ishida, J. L. Johnson, D. J. Whalen, and A. Mesinger. "Detectability of the first cosmic explosions." Monthly Notices of the Royal Astronomical Society 436, no. 2 (October 16, 2013): 1555–63. http://dx.doi.org/10.1093/mnras/stt1680.

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Smartt, Stephen J. "Cosmic explosions in the young Universe." Nature 491, no. 7423 (October 31, 2012): 205–6. http://dx.doi.org/10.1038/nature11643.

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Melott, Adrian L., and Brian C. Thomas. "From Cosmic Explosions to Terrestrial Fires?" Journal of Geology 127, no. 4 (July 2019): 475–81. http://dx.doi.org/10.1086/703418.

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Wheeler, J. Craig. "Astrophysical explosions: from solar flares to cosmic gamma-ray bursts." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 370, no. 1960 (February 13, 2012): 774–99. http://dx.doi.org/10.1098/rsta.2011.0351.

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Astrophysical explosions result from the release of magnetic, gravitational or thermonuclear energy on dynamical time scales, typically the sound-crossing time for the system. These explosions include solar and stellar flares, eruptive phenomena in accretion discs, thermonuclear combustion on the surfaces of white dwarfs and neutron stars, violent magnetic reconnection in neutron stars, thermonuclear and gravitational collapse supernovae and cosmic gamma-ray bursts, each representing a different type and amount of energy release. This paper summarizes the properties of these explosions and describes new research on thermonuclear explosions and explosions in extended circumstellar media. Parallels are drawn between studies of terrestrial and astrophysical explosions, especially the physics of the transition from deflagration-to-detonation.
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Dissertations / Theses on the topic "Cosmic Explosions"

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Soderberg, Alicia Margarita Phinney E. Sterl Kulkarni S. R. "The many facets of cosmic explosions /." Diss., Pasadena, Calif. : California Institute of Technology, 2007. http://resolver.caltech.edu/CaltechETD:etd-05252007-140338.

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Berger, Edo. "Cosmic Explosions: The Beasts and Their Lair." Thesis, Boca Raton, Fla. : Dissertation.Com, 2004. https://thesis.library.caltech.edu/1892/2/intro.pdf.

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The diversity of stellar death is revealed in the energy, velocity and geometry of the explosion debris ("ejecta"). Using multi-wavelength observations of gamma-ray burst (GRB) afterglows I show that GRBs, arising from the death of massive stars, are marked by relativistic, collimated ejecta ("jets") with a wide range of opening angles. I further show that the jet opening angles are strongly correlated with the isotropic-equivalent kinetic energies, such that the true relativistic energy of GRBs is nearly standard, with a value of few times 10^51 erg. A geometry-independent analysis which relies on the simple non-relativistic dynamics of GRBs at late time confirms these inferences. Still, the energy in the highest velocity ejecta, which give rise to the prompt gamma-ray emission, is highly variable. These results suggest that various cosmic explosions are powered by a common energy source, an "engine" (possibly an accreting stellar-mass black hole), with their diverse appearances determined solely by the variable high velocity output. On the other hand, using radio observations I show that local type Ibc core-collapse supernovae generally lack relativistic ejecta and are therefore not powered by engines. Instead, the highest velocity debris in these sources, typically with a velocity lower than 100,000 km/sec, are produced in the (effectively) spherical ejection of the stellar envelope. The relative rates of engine- and collapse-powered explosions suggest that the former account for only a small fraction of the stellar death rate. Motivated by the connection of GRBs to massive stars, and by their ability to overcome the biases inhenert in current galaxy surveys, I investigate the relation between GRB hosts and the underlying population of star-forming galaxies. Using the first radio and submillimeter observations of GRB hosts, I show that some are extreme starburst galaxies with the bursts directly associated with the regions of most intense star formation. I suggest, by comparison to other well-studied samples, that GRBs preferentially occur in sub-luminous, low mass galaxies, undergoing the early stages of a starburst process. If confirmed with future observations, this trend will place GRBs in the forefront of star formation and galaxy evolution studies.
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Berger, Edo Harrison Fiona A. "Cosmic explosions : the beasts and their lair /." Diss., Pasadena, Calif. : California Institute of Technology, 2004. http://resolver.caltech.edu/CaltechETD:etd-05202004-165422.

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Thesis (Ph. D.)--PQ# 3203853.
Paper copy has xvii, 311 leaves because the type-face is larger; chapter numbers are different, also, but the contents are the same; no color in paper copy. Includes bibliographical references.
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Frohmaier, Christopher M. "The rate of cosmic thermonuclear explosions in the Local Universe." Thesis, University of Southampton, 2017. https://eprints.soton.ac.uk/416901/.

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This thesis investigates the volumetric rates of thermonuclear supernovae (SNe) in the Palomar Transient Factory (PTF). SN rates are a measure of how frequently stellar explosions occur as a function of cosmological volumes, or host galaxy properties. SNe are powerful cosmological probes; understanding their rates offers insight into the progenitors to the explosion and the astrophysics of galactic chemical evolution. The Palomar Transient Factory was an automated optical sky survey designed for transient discovery. It spectroscopically confirmed ~1900 SNe during the period of 2009-2012. PTF operated with a 3-5 day cadence, and scanned more than 8,000 square degrees of the sky. I quantified the performance of PTF through large scale simulations of transient events. Firstly, ~7 x 106 fake transient events were inserted into real observational images. These 'fakes' were designed to test the real-time transient discovery pipeline. The images were treated identically to a new PTF observation, where the fakes were either recovered or not. Multidimensional grids were created to describe how a transient would be recovered as a function of the fake's brightness and observing conditions. I found that bright fakes (mR < 18:5) were recovered with ~97% efficiency. PTF was 50% complete at mR = 20.3. The recovery efficiency was also strongly dependent on: the limiting magnitude, the image quality, the sky background, and the immediate environment brightness. The second stage of quantifying the performance of PTF was transient specific. Hundreds of millions of SNe Ia light curves were simulated on an artificial night sky. The simulations shared the statistical properties of the single epoch efficiencies. Through aMonte-Carlo simulation of the SNe Ia populations, I derived recovery efficiencies as a function of SNe Ia light curve parameters. A sample of 90 SNe Ia (z<0.09), were compared to the simulation recovery efficiencies. This provided the probability of the SNe passing rigorous quality cuts, and was used as a weighting factor.
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Soderberg, Alicia Margarita. "The Many Facets of Cosmic Explosions." Thesis, 2007. https://thesis.library.caltech.edu/2071/1/main.pdf.

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Over the past few years, long-duration gamma-ray bursts (GRBs) including the subclass of X-ray flashes (XRFs) have been revealed to be a rare variety of Type Ibc supernova (SN Ibc). While all these events result from the death of massive stars, the electromagnetic luminosities of GRBs and XRFs exceed those of ordinary Type Ibc SNe by many orders of magnitude. The observed diversity of stellar death corresponds to large variations in the energy, velocity and geometry of the explosion ejecta. Using multi-wavelength (radio, optical, X-ray) observations of the nearest GRBs, XRFs, and SNe Ibc, I show that GRBs and XRFs couple at least 1048 erg to relativistic material while SNe Ibc typically couple less than 1048 erg to their fastest (albeit non-relativistic) outflows. Specifically, I find that less than 3% of local SNe Ibc show any evidence for association with a GRB or XRF. Interestingly, this dichotomy is not echoed by the properties of their optical SN emission, dominated by the radioactive decay of Nickel-56; I find that GRBs, XRFs, and SNe Ibc show significant overlap in their optical peak luminosity and photospheric velocities. Recently, I identified a new class of GRBs and XRFs that are under-luminous in comparison with the statistical sample of GRBs. Owing to their faint high energy emission, these sub-energetic bursts are only detectable nearby (z < 0.1) and are likely 10 times more common than cosmological GRBs. In comparison with local SNe Ibc and typical GRBs/XRFs, these explosions are intermediate in terms of both volumetric rate and energetics. Yet the essential physical process that causes a dying star to produce a GRB, XRF, or sub-energetic burst, and not just a SN, remains a crucial open question. Progress requires a detailed understanding of ordinary SNe Ibc which will be facilitated with the launch of wide-field optical surveys in the near future.
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Cao, Yi. "Cosmic Explosions: Observations Of Infant Hydrogen-Free Supernovae Towards An Understanding Of Their Parent Systems." Thesis, 2016. https://thesis.library.caltech.edu/9719/1/yi_cao_2016_thesis.pdf.

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Radiation in the first days of supernova explosions contains rich information about physical properties of the exploding stars. In the past three years, I used the intermediate Palomar Transient Factory to conduct one-day cadence surveys, in order to systematically search for infant supernovae. I show that the one-day cadences in these surveys were strictly controlled, that the realtime image subtraction pipeline managed to deliver transient candidates within ten minutes of images being taken, and that we were able to undertake follow-up observations with a variety of telescopes within hours of transients being discovered. So far iPTF has discovered over a hundred supernovae within a few days of explosions, forty-nine of which were spectroscopically classified within twenty-four hours of discovery.

Our observations of infant Type Ia supernovae provide evidence for both the single-degenerate and double-degenerate progenitor channels. On the one hand, a low-velocity Type Ia supernova iPTF14atg revealed a strong ultraviolet pulse within four days of its explosion. I show that the pulse is consistent with the expected emission produced by collision between the supernova ejecta and a companion star, providing direct evidence for the single degenerate channel. By comparing the distinct early-phase light curves of iPTF14atg to an otherwise similar event iPTF14dpk, I show that the viewing angle dependence of the supernova-companion collision signature is probably responsible to the difference of the early light curves. I also show evidence for a dark period between the supernova explosion and the first light of the radioactively-powered light curve. On the other hand, a peculiar Type Ia supernova iPTF13asv revealed strong near-UV emission and absence of iron in the spectra within the first two weeks of explosion, suggesting a stratified ejecta structure with iron group elements confined to the slow-moving part of the ejecta. With its total ejecta mass estimated to exceed the Chandrasekhar limit, I show that the stratification and large mass of the ejecta favor the double-degenerate channel.

In a separate approach, iPTF found the first progenitor system of a Type Ib supernova iPTF13bvn in the pre-explosion HST archival mages. Independently, I used the early-phase optical observations of this supernova to constrain its progenitor radius to be no larger than several solar radii. I also used its early radio detections to derive a mass loss rate of 3e-5 solar mass per year for the progenitor right before the supernova explosion. These constraints on the physical properties of the iPTF13bvn progenitor provide a comprehensive data set to test Type Ib supernova theories. A recent HST revisit to the iPTF13bvn site two years after the supernova explosion has confirmed the progenitor system.

Moving forward, the next frontier in this area is to extend these single-object analyses to a large sample of infant supernovae. The upcoming Zwicky Transient Facility with its fast survey speed, which is expected to find one infant supernova every night, is well positioned to carry out this task.

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Books on the topic "Cosmic Explosions"

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Marcaide, Juan-María, and Kurt W. Weiler, eds. Cosmic Explosions. Berlin, Heidelberg: Springer Berlin Heidelberg, 2005. http://dx.doi.org/10.1007/b137830.

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Extreme explosions: Supernovae, hypernovae, magnetars, and other unusual cosmic blasts. New York: Springer, 2014.

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October Astrophysics Conference (10th 1999 College Park, Md.). Cosmic explosions: Tenth Astrophysics Conference, College Park, Maryland, 11-13 October 1999. Edited by Holt Stephen S and Zhang William W. Melville, N.Y: AIP, 2000.

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Narlikar, Jayant Vishnu. The cosmic explosion: Science fiction. New Delhi: Sahitya Akademi, 1992.

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Kurt Weiler,J. M. Marcaide. Cosmic Explosions. Springer, 2008.

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Cosmic Explosions in Three Dimensions. Cambridge University Press, 2007.

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Höflich, Peter, Pawan Kumar, and J. Craig Wheeler, eds. Cosmic Explosions in Three Dimensions. Cambridge University Press, 2004. http://dx.doi.org/10.1017/cbo9780511536236.

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Soderberg, Alicia. The Many Facets of Cosmic Explosions. Dissertation.Com, 2007.

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Berger, Edo. Cosmic Explosions: The Beasts And Their Lair. Dissertation.com, 2004.

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Weiler, Kurt, and J. M. Marcaide. Cosmic Explosions: On the 10th Anniversary of SN1993J. Springer, 2014.

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Book chapters on the topic "Cosmic Explosions"

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Kaisig, M., G. Rüdiger, and H. W. Yorke. "The Alpha-Effect by Supernova Explosions." In The Cosmic Dynamo, 389–93. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-0772-3_71.

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Bravo, E., and D. García-Senz. "Asymmetrical Delayed Detonation from a 3D Hydrosimulation of a White Dwarf Explosion." In Cosmic Chemical Evolution, 220. Dordrecht: Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-010-0452-7_28.

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Dorman, Lev I. "Applications of the Radiocarbon Coupling Function Method to Investigations of Planetary Mixing and Exchange Processes; Influence of H-Bomb Explosions on the Environment; Cosmic Ray Variations in the Past." In Astrophysics and Space Science Library, 671–719. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-2113-8_17.

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Wheeler, J. C. "Three-dimensional explosions." In Cosmic Explosions in Three Dimensions, 373–83. Cambridge University Press, 2004. http://dx.doi.org/10.1017/cbo9780511536236.042.

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Wang, L. "Supernova explosions: lessons from spectropolarimetry." In Cosmic Explosions in Three Dimensions, 17–29. Cambridge University Press, 2004. http://dx.doi.org/10.1017/cbo9780511536236.002.

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Andersson, Nils. "Cosmic fireworks." In Gravitational-Wave Astronomy, 508–40. Oxford University Press, 2019. http://dx.doi.org/10.1093/oso/9780198568032.003.0020.

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The simulation of matter in general relativity, be it for neutron star mergers or core collapse, is discussed. State-of-the-art simulations for the dynamical bar-mode instability and neutron star merges are summarized. The inclusion of magnetic field is considered and key issues like the magnetorotational instability are explored. General gravitational collapse is discussed, and the progress toward the simulations of explosions in core-collapse studies is explained.
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Wheeler, J. C. "3-D explosions: a meditation on rotation (and magnetic fields)." In Cosmic Explosions in Three Dimensions, 3–14. Cambridge University Press, 2004. http://dx.doi.org/10.1017/cbo9780511536236.001.

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Filippenko, A. V., and D. C. Leonard. "Spectropolarimetric observations of supernovae." In Cosmic Explosions in Three Dimensions, 30–42. Cambridge University Press, 2004. http://dx.doi.org/10.1017/cbo9780511536236.003.

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Hamuy, M. "Observed and physical properties of Type II plateau supernovae." In Cosmic Explosions in Three Dimensions, 43–49. Cambridge University Press, 2004. http://dx.doi.org/10.1017/cbo9780511536236.004.

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Clocchiatti, A., B. Leibundgut, J. Spyromilio, S. Benetti, E. Cappellaro, M. Turatto, and M. M. Phillips. "SN 1997B and the different types of Type Ic supernovae." In Cosmic Explosions in Three Dimensions, 50–56. Cambridge University Press, 2004. http://dx.doi.org/10.1017/cbo9780511536236.005.

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Conference papers on the topic "Cosmic Explosions"

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Trimble, Virginia. "The first explosions." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291692.

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Aldering, Greg. "Type Ia supernovae & cosmic acceleration." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291697.

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MacFadyen, A. I. "Stellar explosions powered by black hole accretion." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291718.

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Nomoto, Ken’ichi. "Type Ia supernovae: Progenitors and evolution with redshift." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291694.

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Hillebrandt, Wolfgang. "Type Ia supernova explosion models: Homogeneity versus diversity." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291695.

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Suntzeff, Nicholas B. "The observations of Type Ia supernovae." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291696.

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Li, W. D. "A high peculiarity rate for Type Ia SNe." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291699.

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Dyer, Kristy K. "New models for X-ray synchrotron radiation from the remnant of supernova 1006 AD." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291700.

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Dupke, Renato A. "Constraining SN Ia models using X-ray spectra of clusters of galaxies." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291701.

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Li, W. D. "The Lick Observatory Supernova Search." In The tenth astrophysics conference: Cosmic explosions. AIP, 2000. http://dx.doi.org/10.1063/1.1291702.

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Reports on the topic "Cosmic Explosions"

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Fryer, Christopher Lee, Stefano Gandolfi, Przemyslaw R. Wozniak, Joseph Allen Carlson, Aaron Joseph Couture, Joshua C. Dolence, Wesley Paul Even, et al. Nucleosynthesis Probes of Cosmic Explosions. Office of Scientific and Technical Information (OSTI), March 2020. http://dx.doi.org/10.2172/1603951.

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