Discovery of the infrared counterpart of CXOUJ174437.3-323222 in the field of IGR J17448-3232: a blazar candidate viewed through the Galactic Centre?
dc.contributor.author | Curran, Peter | |
dc.contributor.author | Chaty, S. | |
dc.contributor.author | Zurita Heras, J. | |
dc.contributor.author | Tomsick, J. | |
dc.contributor.author | Maccarone, T. | |
dc.date.accessioned | 2017-01-30T14:37:14Z | |
dc.date.available | 2017-01-30T14:37:14Z | |
dc.date.created | 2015-03-03T03:50:59Z | |
dc.date.issued | 2011 | |
dc.identifier.citation | Curran, P. and Chaty, S. and Zurita Heras, J. and Tomsick, J. and Maccarone, T. 2011. Discovery of the infrared counterpart of CXOUJ174437.3-323222 in the field of IGR J17448-3232: a blazar candidate viewed through the Galactic Centre?. Monthly Notices of the Royal Astronomical Society: Letters. 417: pp. L26-L30. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/39816 | |
dc.identifier.doi | 10.1111/j.1745-3933.2011.01113.x | |
dc.description.abstract |
We present our near-infrared ESO-NTTKS band observations of the field of IGRJ17448-3232which show no extended emission consistent with the supernova remnant (SNR), but in whichwe identify a new counterpart, also visible in Spitzer images up to 24 µm, at the position of theX-ray point source, CXOUJ174437.3-323222. Multiwavelength spectral modelling showsthat the data are consistent with a reddened and absorbed single power law over 5 orders ofmagnitude in frequency. This implies non-thermal, possibly synchrotron emission that rendersthe previous identification of this source as a possible pulsar, and its association to the SNR,unlikely; we instead propose that the emission may be due to a blazar viewed through theplane of the Galaxy. | |
dc.publisher | Wiley-Blackwell Publishing Ltd. | |
dc.relation.uri | http://mnrasl.oxfordjournals.org/content/417/1/L26.full.pdf+html | |
dc.subject | radiation mechanisms: non-thermal | |
dc.subject | X-rays: individual: IGRJ17448-3232 | |
dc.subject | infrared: general | |
dc.subject | X-rays: individual: - CXOUJ174437.3-323222 | |
dc.title | Discovery of the infrared counterpart of CXOUJ174437.3-323222 in the field of IGR J17448-3232: a blazar candidate viewed through the Galactic Centre? | |
dc.type | Journal Article | |
dcterms.source.volume | 417 | |
dcterms.source.startPage | L26 | |
dcterms.source.endPage | L30 | |
dcterms.source.issn | 1745-3925 | |
dcterms.source.title | Monthly Notices of the Royal Astronomical Society: Letters | |
curtin.accessStatus | Open access via publisher |