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pro vyhledávání: '"Z. F. Proulx"'
Autor:
Frederic A. Rasio, K. L. Dooley, J. C. Lombardi, Z. F. Proulx, E. M. Theriault, Natalia Ivanova
Publikováno v:
The Astrophysical Journal. 640:441-458
(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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::04339d5e044c4fc32591e83be2c55d68
https://doi.org/10.1086/499938
https://doi.org/10.1086/499938
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d7855c34e4183a18e912881087902b37
