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19 April 2024
 
  » arxiv » 1011.3295

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Identification of a Population of X-ray Emitting Massive Stars in the Galactic Plane
G. E. Anderson ; B. M. Gaensler ; D. L. Kaplan ; B. Posselt ; P. O. Slane ; S. S. Murray ; J. C. Mauerhan ; R. A. Benjamin ; C. L. Brogan ; D. Chakrabarty ; J. J. Drake ; J. E. Drew ; J. E. Grindlay ; J. Hong ; T. J. W. Lazio ; J. C. Lee ; D. T. H. Steeghs ; M. H. van Kerkwijk ;
Date 15 Nov 2010
AbstractWe present X-ray, infrared, optical and radio observations of four previously unidentified Galactic plane X-ray sources, AX J163252-4746, AX J184738-0156, AX J144701-5919 and AX J144547-5931. Detection of each source with the Chandra X-ray Observatory has provided sub-arcsecond localizations, which we use to identify bright infrared counterparts to all four objects. Infrared and optical spectroscopy of these counterparts demonstrate that all four X-ray sources are extremely massive stars, with spectral classifications Ofpe/WN9 (AX J163252-4746), WN7 (AX J184738-0156 = WR121a), WN7-8h (AX J144701-5919) and OIf+ (AX J144547-5931). AX J163252-4746 and AX J184738-0156 are both luminous, hard, X-ray emitters with strong Fe XXV emission lines in their X-ray spectra at ~6.7 keV. The multi-wavelength properties of AX J163252-4746 and AX J184738-0156 are not consistent with isolated massive stars or accretion onto a compact companion; we conclude that their X-ray emission is most likely generated in a colliding-wind binary system. For both AX J144701-5919 and AX J144547-5931, the X-ray emission is an order of magnitude less luminous and with a softer spectrum. These properties are consistent with a colliding-wind binary interpretation for these two sources also, but other mechanisms for the generation of X-rays cannot be excluded. There are many other as yet unidentified X-ray sources in the Galactic plane, with X-ray properties similar to those seen for AX J163252-4746, AX J184738-0156, AX J144701-5919 and AX J144547-5931. This may indicate a substantial population of X-ray-emitting massive stars and colliding-wind binaries in the Milky Way.
Source arXiv, 1011.3295
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