Supernova 2007bi as a pair-instability explosion

A massive star's exit Stars like the Sun end their stellar lives as white dwarfs. Theory predicts a different fate for stars with masses over 140 times that of the Sun (if they exist, which they don't in the Milky Way). When they have evolved to the stage of having oxygen cores the pressur...

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Veröffentlicht in:	Nature (London) 2009-12, Vol.462 (7273), p.624-627
Hauptverfasser:	Gal-Yam, A., Mazzali, P., Ofek, E. O., Nugent, P. E., Kulkarni, S. R., Kasliwal, M. M., Quimby, R. M., Filippenko, A. V., Cenko, S. B., Chornock, R., Waldman, R., Kasen, D., Sullivan, M., Beshore, E. C., Drake, A. J., Thomas, R. C., Bloom, J. S., Poznanski, D., Miller, A. A., Foley, R. J., Silverman, J. M., Arcavi, I., Ellis, R. S., Deng, J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Analysis Chemical properties Cosmochemistry Density Dwarf galaxies Explosions High temperature Humanities and Social Sciences Identification and classification Iron letter Massive stars multidisciplinary Neutron stars Optical properties Science Science (multidisciplinary) Star formation Stars Supernovae Supernovas
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