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

The Hebrew University of Jerusalem, Technion - Israel Institute of Technology

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

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

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

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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",

year = "2012",

doi = "10.1088/1742-6596/337/1/012051",

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note = "5th Bi-Annual Nuclear Physics in Astrophysics, NPA5 ; Conference date: 03-04-2011 Through 08-04-2011",

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AU - Idan, Irit

AU - Shaviv, Nir J.

AU - Shaviv, Giora

PY - 2012

Y1 - 2012

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.

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U2 - 10.1088/1742-6596/337/1/012051

DO - 10.1088/1742-6596/337/1/012051

M3 - مقالة من مؤنمر

SN - 1742-6588

VL - 337

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 1

M1 - 012051

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

All Science Journal Classification (ASJC) codes

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