The First Stellar Explosions: Theoretical Light Curves and Spectra of Pair-Instability Supernovae

Details The First Stellar Explosions: Theoretical Light Curves and Spectra of Pair-Instability Supernovae The First Stellar Explosions: Theoretical Light Curves and Spectra of Pair-Instability Supernovae

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..990..263k&link_type=abstract

FIRST STARS III: First Stars II Conference. AIP Conference Proceedings, Volume 990, pp. 263-267 (2008).

Physics

3

Supernovae, Star Formation, Population Iii Stars, Radiative Transfer, Scattering, Mass Loss And Stellar Winds

Scientific paper

The flrst generation of stars likely consisted of massive objects (M<100 Msolar) which suffered minimal mass loss, setting the stage for an impressive first generation of stellar explosions. For the initial mass range (140

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