King, A.R.; Schenker, K.; Kolb, U. and Davies, M.B.
|DOI (Digital Object Identifier) Link:||http://doi.org/10.1046/j.1365-8711.2001.04002.x|
|Google Scholar:||Look up in Google Scholar|
We show that the usual picture of supersoft X-ray binary evolution as driven by conservative thermal time-scale mass transfer cannot explain the short orbital periods of RX J0537.7–7034 (3.5 h) and 1E 0035.4–7230 (4.1 h). Non-conservative evolution may produce such periods, but requires very significant mass loss, and is highly constrained.
|Item Type:||Journal Article|
|Keywords:||binaries; close; stars; evolution; 1E 0035.4–7230; RX J0537.7–7034; X-rays|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 6827 not found.|
|Date Deposited:||04 Jul 2006|
|Last Modified:||04 Oct 2016 09:51|
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