TY - JOUR
T1 - The fate of a WD accreting H-rich material at high rates
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.
UR - http://www.scopus.com/inward/record.url?scp=84857970370&partnerID=8YFLogxK
U2 - 10.1088/1742-6596/337/1/012051
DO - 10.1088/1742-6596/337/1/012051
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AN - SCOPUS:84857970370
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 -