Are the precursors of type IA supernovae double degenerate mergers?

Lilia Ferrario*

*Corresponding author for this work

    Research output: Contribution to journalConference articlepeer-review

    2 Citations (Scopus)

    Abstract

    I argue that the observational evidence for white dwarf-white dwarf mergers supports the view that they give rise to ultra-massive white dwarfs or neutron stars through accretion induced collapse. The implications for the progenitors of Type Ia SNe are discussed.

    Original languageEnglish
    Pages (from-to)111-112
    Number of pages2
    JournalRevista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
    Volume20
    DOIs
    Publication statusPublished - 2004
    EventIAU Colloquium 194 - Compact Binaries in the Galaxy and Beyond - La Paz, B.C. Sur, Mexico
    Duration: 17 Nov 200322 Nov 2003

    Fingerprint

    Dive into the research topics of 'Are the precursors of type IA supernovae double degenerate mergers?'. Together they form a unique fingerprint.

    Cite this