Black Hole Formation in X-Ray Binaries: The Case of XTE J1118+480.

التفاصيل البيبلوغرافية
العنوان: Black Hole Formation in X-Ray Binaries: The Case of XTE J1118+480.
المؤلفون: Fragos, T., Willems, B., Ivanova, N., Kalogera, V.
المصدر: AIP Conference Proceedings; 8/21/2007, Vol. 924 Issue 1, p673-676, 4p, 1 Chart, 3 Graphs
مصطلحات موضوعية: SUPERMASSIVE black holes, X-ray binaries, STAR formation, BINARY stars, ANGULAR momentum (Nuclear physics), ASTROPHYSICS
مستخلص: In recent years, an increasing number of proper motions have been measured for Galactic X-ray binaries. When supplemented with accurate determinations of the component masses, orbital period, and donor luminosity and effective temperature, these kinematical constraints harbor a wealth of information on the systems’ past evolution. The constraints on compact object progenitors and kicks derived from this are of immense value for understanding compact object formation and exposing common threads and fundamental differences between black hole and neutron star formation. Here, we present the results of such an analysis for the black hole X-ray binary XTE J1118+480. We present results from modeling the mass transfer phase, following the motion in the Galaxy back to the birth site of the black hole, and examining the dynamics of symmetric and asymmetric core-collapses of the black hole progenitor. © 2007 American Institute of Physics [ABSTRACT FROM AUTHOR]
Copyright of AIP Conference Proceedings is the property of American Institute of Physics and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
قاعدة البيانات: Complementary Index
الوصف
تدمد:0094243X
DOI:10.1063/1.2774927