Auswahl der wissenschaftlichen Literatur zum Thema „Stellar feedbacks“
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Zeitschriftenartikel zum Thema "Stellar feedbacks"
Ciardi, B. „Inhomogeneous reionization regulated by radiative and stellar feedbacks“. Astronomical & Astrophysical Transactions 20, Nr. 1 (Juni 2001): 177–82. http://dx.doi.org/10.1080/10556790108208210.
Der volle Inhalt der QuelleEkström, Sylvia, Georges Meynet, Cyril Georgy, José Groh, Arthur Choplin und Hanfeng Song. „Massive star evolution: feedbacks in low-Z environment“. Proceedings of the International Astronomical Union 14, S344 (August 2018): 153–60. http://dx.doi.org/10.1017/s1743921318007238.
Der volle Inhalt der QuelleCiardi, B., A. Ferrara, F. Governato und A. Jenkins. „Inhomogeneous reionization of the intergalactic medium regulated by radiative and stellar feedbacks“. Monthly Notices of the Royal Astronomical Society 314, Nr. 3 (21.05.2000): 611–29. http://dx.doi.org/10.1046/j.1365-8711.2000.03365.x.
Der volle Inhalt der QuelleDekel, Avishai, Nir Mandelker, Frederic Bournaud, Daniel Ceverino, Yicheng Guo und Joel Primack. „Clump survival and migration in VDI galaxies: an analytical model versus simulations and observations“. Monthly Notices of the Royal Astronomical Society 511, Nr. 1 (14.01.2022): 316–40. http://dx.doi.org/10.1093/mnras/stab3810.
Der volle Inhalt der QuelleLocci, Daniele, Antonino Petralia, Giuseppina Micela, Antonio Maggio, Angela Ciaravella und Cesare Cecchi-Pestellini. „Extreme-ultraviolet- and X-Ray-driven Photochemistry of Gaseous Exoplanets“. Planetary Science Journal 3, Nr. 1 (01.01.2022): 1. http://dx.doi.org/10.3847/psj/ac3f3c.
Der volle Inhalt der QuelleFierlinger, Katharina M., Andreas Burkert, Evangelia Ntormousi, Peter Fierlinger, Marc Schartmann, Alessandro Ballone, Martin G. H. Krause und Roland Diehl. „Stellar feedback efficiencies: supernovae versus stellar winds“. Monthly Notices of the Royal Astronomical Society 456, Nr. 1 (17.12.2015): 710–30. http://dx.doi.org/10.1093/mnras/stv2699.
Der volle Inhalt der QuelleForget, F., und J. Leconte. „Possible climates on terrestrial exoplanets“. Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 372, Nr. 2014 (28.04.2014): 20130084. http://dx.doi.org/10.1098/rsta.2013.0084.
Der volle Inhalt der QuelleHerbst, Konstantin, John Lee Grenfell, Miriam Sinnhuber, Heike Rauer, Bernd Heber, Saša Banjac, Markus Scheucher et al. „A new model suite to determine the influence of cosmic rays on (exo)planetary atmospheric biosignatures“. Astronomy & Astrophysics 631 (31.10.2019): A101. http://dx.doi.org/10.1051/0004-6361/201935888.
Der volle Inhalt der QuelleD'Antona, Francesca. „Stellar evolution and feedback connections to stellar dynamics“. Proceedings of the International Astronomical Union 2, Nr. 14 (August 2006): 430–31. http://dx.doi.org/10.1017/s1743921307011222.
Der volle Inhalt der QuelleIvanova, Nataliya M. „Stellar dynamics and feedback connections to stellar evolution“. Proceedings of the International Astronomical Union 2, Nr. 14 (August 2006): 432–33. http://dx.doi.org/10.1017/s1743921307011234.
Der volle Inhalt der QuelleDissertationen zum Thema "Stellar feedbacks"
Maillard, Vincent. „Modèle des fronts de photoevaporation dans les régions de formation d'étoiles“. Electronic Thesis or Diss., Université Paris sciences et lettres, 2023. http://www.theses.fr/2023UPSLO003.
Der volle Inhalt der QuelleThe conditions of formation of stars is a fundamental question of astrophysics. The star formation rate (SFR) is linked to the mass of molecular gas by the Schmidt-Kennicutt relation. However, a star applies some feedbacks on its parent cloud in the form of winds, jets and radiation. They sweep their environment, destroying other star formation sites, but can also compress and destabilize them, triggering the formation of new stars. My thesis focused on the radiative feedback, which is vastly dominated by the one of massive stars. It creates an expanding region where the gas is ionized close to the star, followed by a region where the chemistry is dominated by photons capable of dissociating molecular hydrogen (photodissociation region, or PDR) which includes a layer of atomic hydrogen, which is too hot to form stars. Its width informs us about the fraction of gaz unable to form stars. Numerous models describe the physics and chemistry of PDRs by looking for a stationary state, and neglecting the gas dynamics. However, new observations made by Hershel in excited CO, and by the Atacama Large Millimeter Array (ALMA) in CH+ and SH+ have changed the stationary vision of PDR structure by highlighting the role of the gas dynamics. The edge of clouds is found to be a high-pressure environment, which is strongly correlated to the impinging UV field intensity. The photo-evaporation mechanism is capable of reproducing those features: with the high-speed evaporation of hot ionized gas, the rocket effect makes a pressure wave propagate inside the cloud, explaining the high pressures observed. By the erosion of the cloud, the border withe the ionized medium, the ionization front (IF) advances into the neutral medium. PDR models have to be updated to take into account the propagation of the IF.We built a semi-analytical model of the transition between atomic and molecular gas (H/H2) including the advancing IF. We obtained that the width of the atomic region is reduced compared to static models. It can also disappear if the IF velocity exceeds a threshold value, leading to the merging of the IF and the H/H2 transition. We found analytical formulas to estimate this threshold as well as the total column density of atomic H. By comparing our theory to PDRs observations, we showed that the dynamical effects are strong, especially in the case of weakly illuminated PDRs such as the Horsehead.To prepare for the JWST observations of H2, we have implemented the computation of H2 levels in the Hydra code, which is a hydro-dynamic, time dependent code that models the physics and chemistry of photo-evaporating PDRs. The precedent study allowed to conclude that dynamical effects bring some H2 in a hotter and more illuminated region. The reduction of the IF-H/H2 distance reduces the intensity absorbed by dust, which is then converted to UV-pumping of H2 (amplification by a factor 6 for the Orion Bar, but not efficient in the Horsehead).In addition, we studied ALMA observations of the Horsehead with high spatial resolution. They show a great proximity between the IF and the CO line emission, usually present deep in the cloud. We find an upper limit of a few hundred astronomical units for the width of the atomic region. We find that isobaric, static and stationary Meudon PDR models reproduce the width of the atomic region within the limit found, and so does the dynamical models. These observations therefore do not allow us ton constrain dynamical effects.We performed a study on high spectral resolution observations of rotation-vibration lines of H2 made by the IGRINS spectrograph. We show that the line ratios do not constrain well the physical conditions, but that the population of the states of H2 are much influenced by relaxation rates induced by collisions, unlike the classical picture of a cascade mainly dominated by radiation after the UV pumping
Rogers, Hazel Claire. „Feedback from winds and supernovae in massive stellar clusters“. Thesis, University of Leeds, 2013. http://etheses.whiterose.ac.uk/6858/.
Der volle Inhalt der QuelleGiarrusso, Daniele. „Properties of the galactic-scale gas circulation generated by stellar feedback“. Master's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/20942/.
Der volle Inhalt der QuelleRey, Raposo Ramon. „The interplay between stellar feedback and galactic environment in molecular clouds“. Thesis, University of Exeter, 2015. http://hdl.handle.net/10871/21022.
Der volle Inhalt der QuelleSmith, Matthew Carey. „Modelling star formation and stellar feedback in numerical simulations of galaxy formation“. Thesis, University of Cambridge, 2018. https://www.repository.cam.ac.uk/handle/1810/277830.
Der volle Inhalt der QuelleJose, Jessy, Jinyoung S. Kim, Gregory J. Herczeg, Manash R. Samal, John H. Bieging, Michael R. Meyer und William H. Sherry. „STAR FORMATION IN W3—AFGL 333: YOUNG STELLAR CONTENT, PROPERTIES, AND ROLES OF EXTERNAL FEEDBACK“. IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621216.
Der volle Inhalt der QuelleLochhaas, Cassandra Derrick. „Stellar Feedback in Galaxies, Its Impact on the Circumgalactic Medium, and the Importance of Radiative Cooling“. The Ohio State University, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=osu1562676332648711.
Der volle Inhalt der QuelleGrisdale, Kearn. „The role of stellar feedback on the structure of the ISM and star formation in galaxies“. Thesis, University of Surrey, 2017. http://epubs.surrey.ac.uk/841384/.
Der volle Inhalt der QuelleDECATALDO, DAVIDE. „The Effect of Stellar and Quasar Feedback on the Interstellar Medium: Structure and Lifetime of Molecular Clouds“. Doctoral thesis, Scuola Normale Superiore, 2020. http://hdl.handle.net/11384/90712.
Der volle Inhalt der QuelleSerrano, Medina Sac Nicte Xiomara [Verfasser]. „Radio emission from massive Young Stellar Objects and their surroundings : Characterization and feedback / Sac Nicte Xiomara Serrano Medina“. Bonn : Universitäts- und Landesbibliothek Bonn, 2020. http://d-nb.info/1221668978/34.
Der volle Inhalt der QuelleBücher zum Thema "Stellar feedbacks"
Emerick, Andrew James. Stellar Feedback and Chemical Evolution In Dwarf Galaxies. [New York, N.Y.?]: [publisher not identified], 2019.
Den vollen Inhalt der Quelle findenDAEC Workshop (3rd 1992 Observatoire de Paris-Meudon). The feedback of chemical evolution on the stellar content of galaxies: Proceedings of the 3rd DAEC Workshop, Observatoire de Paris/Meudon October 12-16, 1992. Meudon, France: Imprimerie de l'Observatoire de Paris, Section Meudon, 1992.
Den vollen Inhalt der Quelle findenHoelscher, Jason A. Art as Information Ecology. Duke University Press, 2021. http://dx.doi.org/10.1215/9781478021681.
Der volle Inhalt der QuelleBuchteile zum Thema "Stellar feedbacks"
Ristikangas, Vesa, und Tapani Rinne. „Feedback puts wings on development“. In Stellar Management Teams, 111–23. Abingdon, Oxon ; New York, NY : Routledge, 2018.: Routledge, 2018. http://dx.doi.org/10.4324/9781351244114-14.
Der volle Inhalt der QuelleLetokhov, Vladilen S. „Noncoherent Feedback in Space Masers and Stellar Lasers“. In Amazing Light, 409–43. New York, NY: Springer New York, 1996. http://dx.doi.org/10.1007/978-1-4612-2378-8_41.
Der volle Inhalt der QuelleFender, Rob, und Teo Muñoz-Darias. „The Balance of Power: Accretion and Feedback in Stellar Mass Black Holes“. In Astrophysical Black Holes, 65–100. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-19416-5_3.
Der volle Inhalt der QuelleBastian, Morten, und Andreas Mühling. „Erste Schritte zur automatisierten Generation von Items in einem webbasierten Tracingsystem“. In Die Zukunft des MINT-Lernens – Band 1, 193–210. Berlin, Heidelberg: Springer Berlin Heidelberg, 2022. http://dx.doi.org/10.1007/978-3-662-66131-4_12.
Der volle Inhalt der Quelle„Stellar Feedback“. In Star Formation, 121–40. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813142046_0008.
Der volle Inhalt der QuelleLoeb, Abraham, und Steven R. Furlanetto. „Stellar Feedback and Galaxy Formation“. In The First Galaxies in the Universe. Princeton University Press, 2013. http://dx.doi.org/10.23943/princeton/9780691144917.003.0006.
Der volle Inhalt der Quelle„Chapter Six. Stellar Feedback and Galaxy Formation“. In The First Galaxies in the Universe, 174–216. Princeton: Princeton University Press, 2013. http://dx.doi.org/10.1515/9781400845606.174.
Der volle Inhalt der QuelleAkputu, Oryina Kingsley, und Kingsley Friday Attai. „User Experience Measurement“. In Advances in Business Information Systems and Analytics, 250–82. IGI Global, 2021. http://dx.doi.org/10.4018/978-1-7998-3756-5.ch015.
Der volle Inhalt der QuelleKirschhock, Eva-Maria, Miriam Grüning und Miriam Hess. „Mentoring im Praktikum aus der Sicht von Grundschullehramts- studierenden – Wie können nachhaltige Unterrichtsbesprechungen im Praktikum gestaltet werden?“ In Nachhaltige Bildung in der Grundschule, 452–57. Verlag Julius Klinkhardt, 2023. http://dx.doi.org/10.35468/6035-66.
Der volle Inhalt der QuelleKonferenzberichte zum Thema "Stellar feedbacks"
Padilla, Nelson D., Claudia Lagos, Michael Strauss, Sebastian Heinz und Eric Wilcots. „Stellar Disc—Active Nucleus Alignments in the SDSS“. In THE MONSTER’S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS. AIP, 2009. http://dx.doi.org/10.1063/1.3293009.
Der volle Inhalt der QuelleHueckstaedt, Robert, Daniel Whalen, Thomas McConkie, Daniel J. Whalen, Volker Bromm und Naoki Yoshida. „Local Radiative Feedback: The Rise of Early Stellar Populations“. In THE FIRST STARS AND GALAXIES: CHALLENGES FOR THE NEXT DECADE. AIP, 2010. http://dx.doi.org/10.1063/1.3518869.
Der volle Inhalt der QuelleCIARDI, B., und A. FERRARA. „FIR/SUB-MM LINE EMISSION FROM THE FIRST OBJECTS: TESTING THE STELLAR FEEDBACK“. In Implications for Galaxy Formation and Evolution. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811738_0029.
Der volle Inhalt der QuelleIndahl, Briana, Brian Fleming, Dmitry Vorobiev, Dana Chafetz, Jack Williams, Maitland Bowen, Diane Brening et al. „Status and mission operations of the SPRITE 12U CubeSat: a probe of star formation feedback from stellar to galactic scales with far-UV imaging spectroscopy“. In UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXIII, herausgegeben von Oswald H. Siegmund und Keri Hoadley. SPIE, 2023. http://dx.doi.org/10.1117/12.2677737.
Der volle Inhalt der QuelleBerichte der Organisationen zum Thema "Stellar feedbacks"
Li, Richard. LegalOne Stellar Accolade 2023 - China. LegalOne Global Limited, Dezember 2023. http://dx.doi.org/10.62436/a-1702224947429.
Der volle Inhalt der QuelleDudenbostel, Tobias, und David Heckenberg. Bedarfsanalyse Qualifizierungsoffensive. Endbericht an das Bundesministerium für Digitalisierung und Wirtschaftsstandort (BMDW). BMDW - Bundesministerium für Digitalisierung und Wirtschaftsstandort, Juli 2022. http://dx.doi.org/10.22163/fteval.2022.564.
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