An ultraluminous X-ray object with a 2 hour period in M51
dc.contributor.author | Liu, JF | |
dc.contributor.author | Bregman, JN | |
dc.contributor.author | Irwin, J | |
dc.contributor.author | Seitzer, P | |
dc.contributor.other | University of Michigan System | |
dc.contributor.other | University of Michigan | |
dc.contributor.other | University of Alabama Tuscaloosa | |
dc.date.accessioned | 2018-09-14T15:59:08Z | |
dc.date.available | 2018-09-14T15:59:08Z | |
dc.date.issued | 2002-12-20 | |
dc.description.abstract | Ultraluminous X-ray objects (ULXs) are off-nucleus point sources with L-X = 10(39)-10(41) ergs s(-1), but the nature 39 of such systems is largely unidentified. Here we report a 2.1 hr period observed in a Chandra ACIS observation for ULX M51 X-7, which is located on the edge of a young star cluster in the star-forming region in a spiral arm. In two ACIS observations separated by 1 yr, the ULX changed from a high-hard to a low-soft spectral state, in contrast to most Galactic low-mass X-ray binaries. On the basis of its period and spectral behaviors, we suggest that this ULX is a low-mass X-ray binary system, with a dwarf companion of 0.2-0.3 M. and a compact accretor, either a neutron star or a black hole, whose mass is not well constrained. Relativistic beaming effects are likely involved to produce the observed high X-ray luminosities, given its low accretion rate as inferred from a sustainable accretion scenario via Roche lobe overflow. | en_US |
dc.format.mimetype | application/pdf | |
dc.identifier.citation | Liu, J., Bregman, J., Irwin, J., Seitzer, P. (2002): An Ultraluminous X-Ray Object with a 2 Hour Period in M51. The Astrophysical Journal Letters, 581(2). DOI: 10.1086/346101 | |
dc.identifier.doi | 10.1086/346101 | |
dc.identifier.orcid | https://orcid.org/0000-0001-6276-9526 | |
dc.identifier.uri | http://ir.ua.edu/handle/123456789/3866 | |
dc.language | English | |
dc.language.iso | en_US | |
dc.publisher | University of Chicago Press | |
dc.subject | galaxies : individual (M51) | |
dc.subject | X-rays : binaries | |
dc.subject | GALAXIES | |
dc.subject | EVOLUTION | |
dc.subject | CHANDRA | |
dc.subject | Astronomy & Astrophysics | |
dc.title | An ultraluminous X-ray object with a 2 hour period in M51 | en_US |
dc.type | text | |
dc.type | Article |
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