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pro vyhledávání: '"Proulx, Z. F."'
Autor:
Lombardi Jr., J. C., Proulx, Z. F., Dooley, K. L., Theriault, E. M., Ivanova, N., Rasio, F. A.
Publikováno v:
Astrophys.J.640:441-458,2006
(abridged) We report the results of SPH calculations of parabolic collisions between a subgiant or slightly evolved red-giant star and a neutron star (NS). Such collisions are likely to form ultracompact X-ray binaries (UCXBs) observed today in old g
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509511
Publikováno v:
Astrophys.J. 621 (2005) L109-L112
Bright, ultracompact X-ray binaries observed in dense star clusters, such as Galactic globular clusters, must have formed relatively recently, since their lifetimes as persistent bright sources are short (e.g., ~10^8 yr above 10^36 erg/s for a 1.4 Ms
Externí odkaz:
http://arxiv.org/abs/astro-ph/0501617
Autor:
Lombardi, Jr. J. C., Proulx, Z. F., Dooley, K. L., Theriault, E. M., Ivanova, N., Rasio, F. A.
Publikováno v:
Astrophysical Journal; 3/20/2006, Vol. 640 Issue 1, p441-458, 18p
