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The nature of the X-ray transient MAXI J0556-332

Abstract:

Phase-resolved spectroscopy of the newly discovered X-ray transient MAXIJ0556-332 has revealed the presence of narrow emission lines in the Bowen region that most likely arise on the surface of the mass donor star in this low-mass X-ray binary. A period search of the radial velocities of these lines provides two candidate orbital periods (16.43 ± 0.12 and 9.754 ± 0.048h), which differ from any potential X-ray periods reported. Assuming that MAXIJ0556-332 is a relatively high-inclination syste...

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Publication status:
Published

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Journal:
Monthly Notices of the Royal Astronomical Society
Volume:
420
Issue:
4
Pages:
3538-3544
Publication date:
2012-03-01
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Source identifiers:
361967
Language:
English
Keywords:
Pubs id:
pubs:361967
UUID:
uuid:7ad2b098-2652-4544-93d0-e7ca4b962a6f
Local pid:
pubs:361967
Deposit date:
2013-11-16

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