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Artykuły w czasopismach na temat "Galactic emissions"
Grimaldi, Claudio. "Demography of galactic technosignatures". Monthly Notices of the Royal Astronomical Society 500, nr 2 (7.11.2020): 2278–88. http://dx.doi.org/10.1093/mnras/staa3450.
Pełny tekst źródłaOkuda, H., T. Nakagawa, H. Shibai, Y. Doi, K. Mochizuki, Y. Yamashita-Yui, M. Yui, T. Nishimura i F. J. Low. "Diffuse [CII] Emission in the Galaxy". Symposium - International Astronomical Union 169 (1996): 497–98. http://dx.doi.org/10.1017/s0074180900230143.
Pełny tekst źródłaSofue, Yoshiaki. "4.1. Radio continuum and molecular gas in the Galactic center: large-scale structures". Symposium - International Astronomical Union 184 (1998): 161–68. http://dx.doi.org/10.1017/s0074180900084473.
Pełny tekst źródłaAbbasi, R., M. Ackermann, J. Adams, N. Aggarwal, J. A. Aguilar, M. Ahlers, J. M. Alameddine i in. "Searches for Neutrinos from Large High Altitude Air Shower Observatory Ultra-high-energy γ-Ray Sources Using the IceCube Neutrino Observatory". Astrophysical Journal Letters 945, nr 1 (1.03.2023): L8. http://dx.doi.org/10.3847/2041-8213/acb933.
Pełny tekst źródłaMiroshnichenko, Anatoly S. "MWC 314 – A new galactic B[e] supergiant". Symposium - International Astronomical Union 162 (1994): 396–97. http://dx.doi.org/10.1017/s0074180900215489.
Pełny tekst źródłaMacías-Pérez, J. F., R. D. Davies, R. Watson, C. M. Gutierrez i R. Rebolo. "A Characterization of the Diffuse Galactic Emissions at Large Angular Scales Using the Tenerife Data". Advances in Astronomy 2013 (2013): 1–15. http://dx.doi.org/10.1155/2013/780407.
Pełny tekst źródłaGiard, Martin, i Guilaine Lagache. "Galactic emissions: seeing through the Galaxy". Comptes Rendus Physique 4, nr 8 (październik 2003): 901–8. http://dx.doi.org/10.1016/j.crhy.2003.09.009.
Pełny tekst źródłaDesai, Abhishek, Justin Vandenbroucke, Samalka Anandagoda, Jessie Thwaites i M. J. Romfoe. "Constraints on the Origins of the Galactic Neutrino Flux Detected by IceCube". Astrophysical Journal 966, nr 1 (23.04.2024): 23. http://dx.doi.org/10.3847/1538-4357/ad2a5e.
Pełny tekst źródłaYamauchi, S. "Hot Plasma in the Galaxy". Symposium - International Astronomical Union 188 (1998): 47–50. http://dx.doi.org/10.1017/s0074180900114408.
Pełny tekst źródłaFauvet, L., J. F. Macías-Pérez, S. R. Hildebrandt i F. X. Désert. "A Characterization of the Diffuse Galactic Emissions in the Anticenter of the Galaxy". Advances in Astronomy 2013 (2013): 1–8. http://dx.doi.org/10.1155/2013/746020.
Pełny tekst źródłaRozprawy doktorskie na temat "Galactic emissions"
Szabo, Anthony Paul. "High energy emissions for astrophysical objects". Title page, contents and abstract only, 1992. http://web4.library.adelaide.edu.au/theses/09PH/09phs996.pdf.
Pełny tekst źródłaFauvet, Lauranne. "Cosmologie observationnelle avec le satellite Planck : modélisation des émissions galactiques polarisées". Phd thesis, Grenoble, 2010. http://www.theses.fr/2010GRENY032.
Pełny tekst źródłaThis thesis is dedicated to the Cosmic Microwave Background (CMB) anisotropies measurement and to the characterization of the foreground Galactic emissions. This work is in the framework of the Planck satellite data analysis preparation. First, this thesis gives a description of the Big Bang model and of the CMB physics. Then, we present the Archeops, WMAP and PLANCK experiments and their data analysis. Part two is devoted to the description of the diffuse Galactic synchrotron, free-free and thermal dust emissions and to the study of those emissions in the Galactic plane. Using comparison between our simulations and the WMAP, Archeops and IRIS data we are able to provide partial maps of the spatial variations of the dust grain temperature and of the spectral index of the synchrotron and thermal dust emissions. Third part is dedicated to the study of the two main polarized Galactic emissions: synchrotron and thermal dust emissions. We evaluate effective models based on template maps. We also build physical model based on physics for these emissions that is to say shape of the Galactic magnetic field and matter density in our Galaxy. Using maps and Galactic profiles, we compare our simulations of these emissions to the Archeops and WMAP data. Thanks to that we are able to provide for the first time a coherent model of the synchrotron and thermal dust emissions. Then we propose a method to improve the constraints on our model using the PLANCK data. Finally the last part focuses on the angular power spectra of the polarized Galactic emissions. We estimate the contamination due to these foreground emissions on the CMB signal. In addition we propose a method to minimize the contamination of the CMB PLANCK data by the thermal dust emission using masks
Jones, Laurence Richard. "X-ray emission from galactic supernova remnants". Thesis, University of Leicester, 1986. http://hdl.handle.net/2381/35703.
Pełny tekst źródłaCerruti, Matteo. "High-energy emission from active galactic nuclei". Paris 7, 2012. http://www.theses.fr/2012PA077225.
Pełny tekst źródła. In this thesis manuscript we tried to summarize the research work done during the last three years in the high-energy group of the LUTh laboratory, as well as in the H. E. S. S. Collaboration. The project deals with the study of high-energy emission from active galactic nuclei (AGN), where, with high energy, we refer here to X and y-rays. The thesis covers in fact two différent aspects of the physics of AGN, firstly the study of the X-ray emission from Seyfert galaxies (radio-quiet AGN), and then of the y-ray emission from blazars (radio-loud AGN). We start then by providing a short introduction to the scientific context of AGN physics (by present- ing the unified AGN model), as well as of TeV astronomy. In the first part we first describe the problem of the soft-X-ray excess in Seyfert galaxies (Chapter 1), before entering in the details of the study of Suzaku observations of two particular objects (Mrk 509 and Mrk 841, Chapter 2), presenting the data analysis and their modelling. The second part starts with an introduction on the blazar physics (Chapter 3), before showing the results achieved by the H. E. S. S. Telescope array on AGN (Chapter 4). A detailed study has been done on a particular blazar detected at TeV energies (1RXS J101015. 9 - 311909), and is presented in Chapter 5. The following chapters are more theoretical, and discuss the modelling of the observed blazar emis- sion. In particular, in Chapter 6 we discuss the constrains on the synchrotron-self-Compton model, presenting a new numerical algorithm to determine the best-fit solution, while in Chapter 7 we present a new stationary lepto-hadronic code, which can be used to model the blazar emission in leptonic, hadronic and mixed scenarios. In Chapter 8 we present the problem of the spectral break observed in the GeV spectrum of 3C 454. 3, and we model it consistently in an external-inverse-Compton scenario. Finally we present a perspective for the detection of high-redshift sources with the future telescope CTA (Appendix A)
Espey, Brian Russell. "Emission line studies of high redshift AGN". Thesis, University of Cambridge, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.317876.
Pełny tekst źródłaHands, Alex. "Diffuse and discrete sources of galactic X-ray emission". Thesis, University of Leicester, 2004. http://hdl.handle.net/2381/30675.
Pełny tekst źródłaAlves, Marta Isabel Rocha. "Diffuse radio recombination line emission on the galactic plane". Thesis, University of Manchester, 2011. https://www.research.manchester.ac.uk/portal/en/theses/diffuse-radio-recombination-line-emission-on-the-galactic-plane(54655adf-a0da-4f27-86fb-0d8ae43e1e80).html.
Pełny tekst źródłaMak, Wai-ying, i 麥偉瑩. "Very high energy gamma-ray emission from active galactic nuclei". Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1999. http://hub.hku.hk/bib/B31221464.
Pełny tekst źródłaMak, Wai-ying. "Very high energy gamma-ray emission from active galactic nuclei /". Hong Kong : University of Hong Kong, 1999. http://sunzi.lib.hku.hk/hkuto/record.jsp?B20567492.
Pełny tekst źródłaPage, Mathew James. "X-ray evolution and variability of active galactic nuclei". Thesis, University College London (University of London), 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.267655.
Pełny tekst źródłaKsiążki na temat "Galactic emissions"
Aktivna galaktička jezgra: Primer galaksije Mrk 817. Beograd: Zadužbina Andrejević, 2006.
Znajdź pełny tekst źródłaUnited States. National Aeronautics and Space Administration., red. Final technical report: Studies of the evolution of the X-ray emission of clusters of galaxies. [Washington, D.C: National Aeronautics and Space Administration, 1990.
Znajdź pełny tekst źródłaUnited States. National Aeronautics and Space Administration., red. Final technical report: Studies of the evolution of the X-ray emission of clusters of galaxies. [Washington, D.C: National Aeronautics and Space Administration, 1990.
Znajdź pełny tekst źródłaIAU Colloquium (159th 1996 Shanghai, China). Emission lines in active galaxies: New methods and techniques : IAU Colloquim 159 : meeting held in Shanghai, People's Republic of China, 17-20 June 1996. San Francisco, Calif: Astronomical Society of the Pacific, 1997.
Znajdź pełny tekst źródłaVerner, Ekaterina. Fe II emission from HII regions and active galactic nuclei. Toronto: Graduate Department of Astronomy, University of Toronto, 2000.
Znajdź pełny tekst źródłaHartmann, Dap. The Leiden/Dwingeloo survey of galactic neutral hydrogen. Leiden: Sterrewacht Leiden, 1994.
Znajdź pełny tekst źródłaHartmann, Dap. The Leiden/Dwingeloo survey of galactic neutral hydrogen. Leiden: Sterrewacht Leiden, 1995.
Znajdź pełny tekst źródłaJordi, Cepa, red. The emission-line universe: XVIII Canary Islands Winter School of Astrophysics. New York: Cambridge University Press, 2008.
Znajdź pełny tekst źródłaSandford, Scott A. The galactic distribution of aliphatic hydrocarbons in the diffuse interstellar medium. [Washington, D.C: National Aeronautics and Space Administration, 1995.
Znajdź pełny tekst źródłaSandford, Scott A. The galactic distribution of aliphatic hydrocarbons in the diffuse interstellar medium. [Washington, D.C: National Aeronautics and Space Administration, 1995.
Znajdź pełny tekst źródłaCzęści książek na temat "Galactic emissions"
Tavani, Marco. "Binary Pulsar Shock Emissions as Galactic Gamma-Ray Sources". W The Gamma Ray Sky with Compton GRO and SIGMA, 181–95. Dordrecht: Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0067-0_15.
Pełny tekst źródłaNetzer, Hagai. "AGN Emission Lines". W Active Galactic Nuclei, 57–160. Berlin, Heidelberg: Springer Berlin Heidelberg, 1990. http://dx.doi.org/10.1007/978-3-662-39816-6_2.
Pełny tekst źródłaMoore, N. P., J. S. Panesar i A. H. Nelson. "Galactic Dynamo Models". W Multi-Wavelength Continuum Emission of AGN, 486. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-010-9537-2_187.
Pełny tekst źródłaGreen, Richard, Patrick Osmer i Alain Porter. "Quasar Emission — Line Strengths". W Active Galactic Nuclei, 124–25. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0963-2_36.
Pełny tekst źródłaSalter, Chris J., i Robert L. Brown. "Galactic Nonthermal Continuum Emission". W Astronomy and Astrophysics Library, 1–36. New York, NY: Springer New York, 1988. http://dx.doi.org/10.1007/978-1-4612-3936-9_1.
Pełny tekst źródłaStrong, A. W. "Diffuse Galactic Continuum Emission". W The Gamma Ray Sky with Compton GRO and SIGMA, 147–58. Dordrecht: Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0067-0_12.
Pełny tekst źródłaImpey, C. D., C. G. Wynn-Williams i E. E. Becklin. "Infrared Emission from Radio Galaxies". W Active Galactic Nuclei, 404–5. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0963-2_125.
Pełny tekst źródłaMaoz, Dan. "Emission-Line Variability in AGN". W Active Galactic Nuclei, 100–102. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0963-2_25.
Pełny tekst źródłaJunkkarinen, Vesa. "QSO Emission Line Redshift Differences". W Active Galactic Nuclei, 122–23. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0963-2_35.
Pełny tekst źródłaKallman, T. R., J. H. Krolik i B. J. Wilkes. "Quasar Emission Line Profile Modelling". W Active Galactic Nuclei, 131–32. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0963-2_39.
Pełny tekst źródłaStreszczenia konferencji na temat "Galactic emissions"
Digel, Seth W. "Galactic Diffuse Emissions". W THE FIRST GLAST SYMPOSIUM. AIP, 2007. http://dx.doi.org/10.1063/1.2757281.
Pełny tekst źródłaRenzi, Alessandro. "Primordial non-Gaussianity and diffuse Galactic emissions". W Big Bang, Big Data, Big Computers. Trieste, Italy: Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.165.0031.
Pełny tekst źródłaPapavasileiou, Theodora V., Odysseas T. Kosmas i Ioannis Sinatkas. "Modeling simulated emissions from galactic binary stars". W 11TH INTERNATIONAL CONFERENCE ON MATHEMATICAL MODELING IN PHYSICAL SCIENCES. AIP Publishing, 2023. http://dx.doi.org/10.1063/5.0162914.
Pełny tekst źródłaHigdon, J. C. "Theoretical estimates of diffuse galactic γ-ray emissions". W AIP Conference Proceedings Volume 170. AIP, 1988. http://dx.doi.org/10.1063/1.37249.
Pełny tekst źródłaMoskalenko, Igor, G. Johannesson, E. Orlando, Troy Porter i A. W. Strong. "GALPROP Code for Galactic Cosmic Ray Propagation and Associated Photon Emissions". W 35th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0279.
Pełny tekst źródłavon Ballmoos, P. "A distribution for the galactic 26Al and e+e− line emissions". W Gamma-ray line astrophysics. AIP, 1991. http://dx.doi.org/10.1063/1.40928.
Pełny tekst źródłaMoskalenko, Igor, Guðlaugur Jóhannesson i Troy Porter. "GALPROP Code for Galactic Cosmic Ray Propagation and Associated Photon Emissions". W 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0152.
Pełny tekst źródłaMoskalenko, Igor, Gudlaugur Johannesson i Troy Porter. "GALPROP Code for Galactic Cosmic Ray Propagation and Associated Photon Emissions". W 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0111.
Pełny tekst źródłaMoskalenko, Igor. "GALPROP Code for Galactic Cosmic Ray Propagation and Associated Photon Emissions". W The 34th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.236.0492.
Pełny tekst źródłaFauvet, Lauranne, i Juan-Francisco Macias-Pérez. "Preparation to the Planck Analysis: 3D Modelisation of the Polarized Galactic Emissions". W International Workshop on Cosmic Structure and Evolution. Trieste, Italy: Sissa Medialab, 2010. http://dx.doi.org/10.22323/1.097.0016.
Pełny tekst źródłaRaporty organizacyjne na temat "Galactic emissions"
Moskalenko, Igor V., Andrew W. Strong, Seth W. Digel i Troy A. Porter. Developing the Galactic Diffuse Emission Model for the GLAST Large Area Telescope. Office of Scientific and Technical Information (OSTI), kwiecień 2007. http://dx.doi.org/10.2172/903007.
Pełny tekst źródłaPorter, Troy A., Igor V. Moskalenko i Andrew W. Strong. Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field. Office of Scientific and Technical Information (OSTI), sierpień 2006. http://dx.doi.org/10.2172/888781.
Pełny tekst źródłaBaltz, E. Diffuse Inverse Compton and Synchrotron Emission from Dark Matter Annihilations in Galactic Satellites. Office of Scientific and Technical Information (OSTI), kwiecień 2004. http://dx.doi.org/10.2172/826862.
Pełny tekst źródłaWoods, Natasha. Probing the Geometry and Physics of the Emission Region in Active Galactic Nuclei using hard X-ray & Gamma-ray Observations. Office of Scientific and Technical Information (OSTI), sierpień 2010. http://dx.doi.org/10.2172/992928.
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