Rate of WD-WD head-on collisions in isolated triples is too low to explain standard type Ia supernovae

By Toonen S.   Perets H. B.   Hamers A. S.  

Astronomy & Astrophysics, Vol. 610, Iss. issue, 2018-02 ,pp. : A22-A22

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Super-Eddington wind scenario for the progenitors of type Ia supernovae: Accreting He-rich matter onto white dwarfs

By Wang B.   Li Y.   Ma X.   Liu D.-D.   Cui X.   Han Z.  

Astronomy & Astrophysics, Vol. 584, Iss. issue, 2015-11 ,pp. : A37-A37

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Producing Type Iax supernovae from a specific class of helium-ignited WD explosions

By Wang B.   Justham S.   Han Z.  

Astronomy & Astrophysics, Vol. 559, Iss. issue, 2013-11 ,pp. : A94-A94

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The correlation between C/O ratio, metallicity, and the initial WD mass for SNe Ia⋆

By Meng X. C.   Yang W. M.  

Astronomy & Astrophysics, Vol. 531, Iss. issue, 2011-06 ,pp. : A94-A94

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Rotation of surviving companion stars after type Ia supernova explosions in the WD+MS scenario

By Liu Z.-W.   Pakmor R.   Röpke F. K.   Edelmann P.   Hillebrandt W.   Kerzendorf W. E.   Wang B.   Han Z. W.  

Astronomy & Astrophysics, Vol. 554, Iss. issue, 2013-06 ,pp. : A109-A109

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