Population synthesis for double white dwarfs - II. Semi-detached systems: AM CVn stars
A&A, 368 3 (2001) 939-949
Published online: 2001-03-15
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The long-period AM CVn star SDSS J155252.48+32 0150.9
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https://doi.org/10.1111/j.1365-2966.2007.12397.x
ULTRACAM photometry of the ultracompact binaries V407 Vul and HM Cnc
S. C. C. Barros, T. R. Marsh, V. S. Dhillon, et al.Monthly Notices of the Royal Astronomical Society 374 (4) 1334 (2007)
https://doi.org/10.1111/j.1365-2966.2006.11244.x
Hubble Space TelescopeParallaxes of AM CVn Stars and Astrophysical Consequences
G. H. A. Roelofs, P. J. Groot, G. F. Benedict, et al.The Astrophysical Journal 666 (2) 1174 (2007)
https://doi.org/10.1086/520491
The Stability of Double White Dwarf Binaries Undergoing Direct‐Impact Accretion
Patrick M. Motl, Juhan Frank, Joel E. Tohline and Mario C. R. D’SouzaThe Astrophysical Journal 670 (2) 1314 (2007)
https://doi.org/10.1086/522076
On the orbital periods of the AM CVn stars HP Librae and V803 Centauri
G. H. A. Roelofs, P. J. Groot, G. Nelemans, T. R. Marsh and D. SteeghsMonthly Notices of the Royal Astronomical Society 379 (1) 176 (2007)
https://doi.org/10.1111/j.1365-2966.2007.11931.x
Magnetically Driven Explosions of Rapidly Rotating White Dwarfs Following Accretion‐Induced Collapse
L. Dessart, A. Burrows, E. Livne and C. D. OttThe Astrophysical Journal 669 (1) 585 (2007)
https://doi.org/10.1086/521701