The fate of a WD accreting H-rich material at high rates

Irit Idan; Nir J. Shaviv; Giora Shaviv

doi:10.1088/1742-6596/337/1/012051

The fate of a WD accreting H-rich material at high rates

Irit Idan^*
, Nir J. Shaviv
, Giora Shaviv

^*Corresponding author for this work

Racah Institute of Physics

Research output: Contribution to journal › Conference article › peer-review

9 Scopus citations

Abstract

We study a white dwarf (WD) accreting solar-composition material at super-Eddington accretion rates. We find that after many cycles of hydrogen ignition and burning, several large Helium burning flashes expel the accreted envelope, leaving no net mass accumulation. This implies that such a system will not undergo accretion induced collapse.

Original language	English
Article number	012051
Journal	Journal of Physics: Conference Series
Volume	337
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/337/1/012051
State	Published - 2012
Event	5th Bi-Annual Nuclear Physics in Astrophysics, NPA5 - Eilat, Israel Duration: 3 Apr 2011 → 8 Apr 2011

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10.1088/1742-6596/337/1/012051

Cite this

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title = "The fate of a WD accreting H-rich material at high rates",

abstract = "We study a white dwarf (WD) accreting solar-composition material at super-Eddington accretion rates. We find that after many cycles of hydrogen ignition and burning, several large Helium burning flashes expel the accreted envelope, leaving no net mass accumulation. This implies that such a system will not undergo accretion induced collapse.",

author = "Irit Idan and Shaviv, \{Nir J.\} and Giora Shaviv",

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AU - Shaviv, Nir J.

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N2 - We study a white dwarf (WD) accreting solar-composition material at super-Eddington accretion rates. We find that after many cycles of hydrogen ignition and burning, several large Helium burning flashes expel the accreted envelope, leaving no net mass accumulation. This implies that such a system will not undergo accretion induced collapse.

AB - We study a white dwarf (WD) accreting solar-composition material at super-Eddington accretion rates. We find that after many cycles of hydrogen ignition and burning, several large Helium burning flashes expel the accreted envelope, leaving no net mass accumulation. This implies that such a system will not undergo accretion induced collapse.

UR - https://www.scopus.com/pages/publications/84857970370

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T2 - 5th Bi-Annual Nuclear Physics in Astrophysics, NPA5

Y2 - 3 April 2011 through 8 April 2011

ER -

The fate of a WD accreting H-rich material at high rates

Abstract

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