Peculiar type I supernovae - Explosive helium burning in a low-mass accreting white dwarf

Details Peculiar type I supernovae - Explosive helium burning in a low-mass accreting white dwarf Peculiar type I supernovae - Explosive helium burning in a low-mass accreting white dwarf

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..366k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, May 1986, p. 366-372) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, May-June

Astronomy and Astrophysics

Astronomy

3

Helium, Nuclear Fusion, Peculiar Stars, Stellar Luminosity, Supernovae, White Dwarf Stars, Abundance, Stellar Activity, Stellar Mass Ejection

Scientific paper

It is supposed that a peculiar supernova of type I (SN Ip) may result from explosive helium burning in small mass (MWD < 1 M_sun;) helium or carbon-oxygen-helium white dwarfs. Incomplete helium burning may explain as well small velocities and lower luminosities of SN Ip. Differences between SN Ip and SN I spectra may be due to particular properties of explosive helium burning.

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