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An unusual white dwarf star may be a surviving remnant of a subluminous Type Ia supernova

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00481069" target="_blank" >RIV/67985815:_____/17:00481069 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1126/science.aam8378" target="_blank" >http://dx.doi.org/10.1126/science.aam8378</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1126/science.aam8378" target="_blank" >10.1126/science.aam8378</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    An unusual white dwarf star may be a surviving remnant of a subluminous Type Ia supernova

  • Original language description

    Subluminous Type Ia supernovae, such as the Type Iax-class prototype SN 2002cx, are described by a variety of models such as the failed detonation and partial deflagration of an accreting carbon-oxygen white dwarf star or the explosion of an accreting, hybrid carbon-oxygen-neon core. These models predict that bound remnants survive such events with, according to some simulations, a high kick velocity. We report the discovery of a high proper motion, low-mass white dwarf (LP 40-365) that travels at a velocity greater than the Galactic escape velocity and whose peculiar atmosphere is dominated by intermediate-mass elements. Strong evidence indicates that this partially burnt remnant was ejected following a subluminous Type Ia supernova event. This supports the viability of single-degenerate supernova progenitors.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA15-15943S" target="_blank" >GA15-15943S: Modelling and evolution of magnetic fields in hydrogen-rich and polluted white dwarfs</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2017

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Science

  • ISSN

    0036-8075

  • e-ISSN

  • Volume of the periodical

    357

  • Issue of the periodical within the volume

    6352

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    4

  • Pages from-to

    680-683

  • UT code for WoS article

    000407793600033

  • EID of the result in the Scopus database

    2-s2.0-85027890336