Search Results - "Murphy, Laura J"

Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function by Murphy, Laura J, Groh, Jose H, Farrell, Eoin, Meynet, Georges, Ekström, Sylvia, Tsiatsiou, Sophie, Hackett, Alexander, Martinet, Söbastien

“…ABSTRACT The first stars are thought to be one of the dominant sources of hydrogen reionization in the early Universe, with their high luminosities and surface…”
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Grids of stellar models with rotation – V. Models from 1.7 to 120 M⊙ at zero metallicity by Murphy, Laura J, Groh, Jose H, Ekström, Sylvia, Meynet, Georges, Pezzotti, Camila, Georgy, Cyril, Choplin, Arthur, Eggenberger, Patrick, Farrell, Eoin, Haemmerlé, Lionel, Hirschi, Raphael, Maeder, André, Martinet, Sebastién

“…ABSTRACT Understanding the nature of the first stars is key to understanding the early Universe. With new facilities such as James Webb Space Telescope (JWST)…”
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Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function by Murphy, Laura J, Groh, Jose H, Farrell, Eoin, Meynet, Georges, Ekström, Sylvia, Tsiatsiou, Sophie, Hackett, Alexander, Martinet, Sébastien

“…The first stars are thought to be one of the dominant sources of hydrogen reionization in the early Universe, with their high luminosities and surface…”
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Grids of stellar models with rotation: V. Models from 1.7 to 120 Msun at zero metallicity by Murphy, Laura J, Groh, Jose H, Ekstrom, Sylvia, Meynet, Georges, Pezzotti, Camila, Georgy, Cyril, Choplin, Arthur, Eggenberger, Patrick, Farrell, Eoin, Haemmerle, Lionel, Hirschi, Raphael, Maeder, Andre, Martinet, Sebastien

“…Understanding the nature of the first stars is key to understanding the early universe. With new facilities such as JWST we may soon have the first…”
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Grids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004 by Groh, Jose H, Ekström, Sylvia, Georgy, Cyril, Meynet, Georges, Choplin, Arthur, Eggenberger, Patrick, Hirschi, Raphael, Maeder, Andre, Murphy, Laura J, Boian, Ioana, Farrell, Eoin J

“…A&A 627, A24 (2019) The effects of rotation on stellar evolution are particularly important at low metallicity, when mass loss by stellar winds diminishes and…”
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