کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
1769263 | 1020265 | 2006 | 6 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Evolution of X-ray binaries: Achievements and advances
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کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
علوم فضا و نجوم
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چکیده انگلیسی
Three recent developments in the field of formation and evolution of neutron stars and black holes in binaries are addressed:
• The finding that there is a class of neutron stars, formed in interacting binaries, that do not receive kick velocities in their birth events. This finding is particularly important for our understanding of the formation – and formation rates – of double neutron stars. It is argued that these low-kick neutron stars, which tend to have low masses, are formed by a different physical mechanism than the neutron stars that receive large kick velocities at birth.
• The occurrence of velocity kicks in the formation events of stellar black holes.
• The nature of the companions of millisecond X-ray pulsars.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Advances in Space Research - Volume 38, Issue 12, 2006, Pages 2667–2672
Journal: Advances in Space Research - Volume 38, Issue 12, 2006, Pages 2667–2672
نویسندگان
E.P.J. van den Heuvel,