• Corpus ID: 244709119

Slow Accretion of Helium Rich Matter onto C-O White Dwarf: Does Composition of WD Matter?

@inproceedings{Kumar2021SlowAO,
  title={Slow Accretion of Helium Rich Matter onto C-O White Dwarf: Does Composition of WD Matter?},
  author={Harish Kumar and Abhinav Gupta and Siddharth Malu and Shashikant Gupta},
  year={2021}
}
Background: In binary systems, the helium accretion onto carbon-oxygen (CO) white dwarfs (WDs) plays a vital role in many astrophysical scenarios, especially in supernovae type Ia. Moreover, ignition density for accretion rate M ≲ 10 -9 M yr -1 in helium accreting CO white dwarfs decides the triggering mechanism of a supernova explosion which could be either off-centre helium flash or central carbon flash. Objectives: We aim to study the accretion of helium with a slow accretion rate 5 (cid:2) 10… 

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