How the merger of two white dwarfs depends on their mass ratio: orbital stability and detonations at contact

Author： Dan Marius Rosswog Stephan Guillochon James Ramirez-Ruiz Enrico

ISSN： 0035-8711

Source： Monthly Notices of the Royal Astronomical Society, Vol.422, Iss.3, 2012-05, pp. : 2417-2428

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Low-Mass Quark Stars or Quark White Dwarfs

By Alaverdyan G.B. Harutyunyan A.R. Vartanyan Y.L.

Astrophysics, Vol. 44, Iss. 2, 2001-04 ,pp. : 265-275

Springer Publishing Company

Access to resources Recommend Favorite

Local (thick-disc) white dwarfs and the Galactic mass budget

By Fuhrmann K. Chini R. Hoffmeister V. H. Bernkopf J.

Monthly Notices of the Royal Astronomical Society, Vol. 420, Iss. 2, 2012-02 ,pp. : 1423-1428

Oxford University Press

Access to resources Recommend Favorite

Edmund C. Stoner and the Discovery of the Maximum Mass of White Dwarfs

By Nauenberg Michael

Journal for the History of Astronomy, Vol. 39, Iss. 3, 2008-08 ,pp. : 297-312

Science History Publications Ltd.

Access to resources Recommend Favorite

On the Stability of Contact Discontinuity Separating Two Hypersonic Sources

By Myasnikov A.V. Belov N.A.

Astrophysics and Space Science, Vol. 274, Iss. 1-2, 2000-01 ,pp. : 321-326

Springer Publishing Company

Access to resources Recommend Favorite