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Optical identification of IGR J19140+0951
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In't Zand, J. J. M., Jonker, P. G., Nelemans, G., Steeghs, D. (Danny), 1972- and O'Brien, K.. (2006) Optical identification of IGR J19140+0951. Astronomy and Astrophysics, Vol.448 (No.3). pp. 1101-1106. ISSN 0004-6361
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Official URL: http://dx.doi.org/10.1051/0004-6361:20053411
Abstract
IGR J19140+0951 was discovered by INTEGRAL in 2003 in the 4-100 keV band. Observations with INTEGRAL and RXTE provide a tentative identification as a high-mass X-ray binary (HMXB) with a neutron star as accretor. However, an optical counterpart was thus far not established, nor was the presence of a pulsar which is commonly observed in HMXBs. We observed IGR J19140+0951 with Chandra and find the source to be active at a similar flux as previous measurements. The lightcurve shows a marginally significant oscillation at 6.5 ks which requires confirmation. We determine a sub-arcsecond position from the Chandra data and identify the heavily reddened optical counterpart 2MASS 19140422+0952577 in the 2MASS catalog. Optical follow-up observations with the William Herschel Telescope at La Palma exhibit a continuum spectrum coming out of extinction above 7000 Å without strong absorption or emission features. V, I and band photometry point to an optical counterpart with an extinction of . The extinction is consistent with the interstellar value. None of the data reject the suspicion that IGR J19140+0951 is an HMXB with additional circumstellar obscuration around the accretor.
| Item Type: | Journal Article |
|---|---|
| Subjects: | Q Science > QB Astronomy |
| Divisions: | Faculty of Science > Physics |
| Library of Congress Subject Headings (LCSH): | X-ray binaries |
| Journal or Publication Title: | Astronomy and Astrophysics |
| Publisher: | EDP Sciences |
| ISSN: | 0004-6361 |
| Date: | 2006 |
| Volume: | Vol.448 |
| Number: | No.3 |
| Page Range: | pp. 1101-1106 |
| Identification Number: | 10.1051/0004-6361:20053411 |
| Status: | Peer Reviewed |
| Publication Status: | Published |
| Access rights to Published version: | Restricted or Subscription Access |
| Funder: | Nederlandse Organisatie voor Wetenschappelijk Onderzoek [Netherlands Organisation for Scientific Research] (NWO), Smithsonian Astrophysical Observatory |
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| URI: | http://wrap.warwick.ac.uk/id/eprint/49500 |
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