|
|
|
|
LEADER |
03473 am a22004453u 4500 |
001 |
70016 |
042 |
|
|
|a dc
|
100 |
1 |
0 |
|a Anderson, Gemma E.
|e author
|
100 |
1 |
0 |
|a Massachusetts Institute of Technology. Department of Physics
|e contributor
|
100 |
1 |
0 |
|a MIT Kavli Institute for Astrophysics and Space Research
|e contributor
|
100 |
1 |
0 |
|a Chakrabarty, Deepto
|e contributor
|
100 |
1 |
0 |
|a Chakrabarty, Deepto
|e contributor
|
700 |
1 |
0 |
|a Gaensler, B. M.
|e author
|
700 |
1 |
0 |
|a Kaplan, David L.
|e author
|
700 |
1 |
0 |
|a Posselt, Bettina
|e author
|
700 |
1 |
0 |
|a Slane, Patrick O.
|e author
|
700 |
1 |
0 |
|a Murray, Stephen S.
|e author
|
700 |
1 |
0 |
|a Mauerhan, Jon C.
|e author
|
700 |
1 |
0 |
|a Benjamin, Robert A.
|e author
|
700 |
1 |
0 |
|a Brogan, Crystal L.
|e author
|
700 |
1 |
0 |
|a Chakrabarty, Deepto
|e author
|
700 |
1 |
0 |
|a Drake, Jeremy J.
|e author
|
700 |
1 |
0 |
|a Drew, Janet E.
|e author
|
700 |
1 |
0 |
|a Grindlay, Jonathan E.
|e author
|
700 |
1 |
0 |
|a Hong, Jaesub
|e author
|
700 |
1 |
0 |
|a Lazio, T. Joseph W.
|e author
|
700 |
1 |
0 |
|a Lee, Julia C.
|e author
|
700 |
1 |
0 |
|a Steeghs, Danny T. H.
|e author
|
700 |
1 |
0 |
|a van Kerkwijk, Marten H.
|e author
|
245 |
0 |
0 |
|a Identification of A Population of X-ray-emitting Massive Stars in the Galactic Plane
|
260 |
|
|
|b Institute of Physics Publishing,
|c 2012-04-13T15:59:44Z.
|
856 |
|
|
|z Get fulltext
|u http://hdl.handle.net/1721.1/70016
|
520 |
|
|
|a We 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 (CWB) 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 CWB 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 CWBs in the Milky Way.
|
520 |
|
|
|a United States. National Aeronautics and Space Administration (Hubble Fellowship grant 51230.01-A)
|
520 |
|
|
|a Australian Research Council (Federation Fellowship grant FF0561298)
|
520 |
|
|
|a United States. National Aeronautics and Space Administration (NASA Contract No. NAS8-03060)
|
520 |
|
|
|a Science and Technology Facilities Council (Great Britain) (Advanced Fellowship)
|
546 |
|
|
|a en_US
|
655 |
7 |
|
|a Article
|
773 |
|
|
|t Astrophysical Journal
|