Reference : The X-ray light curve of the massive colliding wind Wolf-Rayet + O binary WR 21a
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/197849
The X-ray light curve of the massive colliding wind Wolf-Rayet + O binary WR 21a
English
Gosset, Eric mailto [Université de Liège > > Groupe d'astrophysique des hautes énergies (GAPHE) >]
Nazé, Yaël mailto [Université de Liège > > Groupe d'astrophysique des hautes énergies (GAPHE) >]
1-May-2016
Astronomy and Astrophysics
EDP Sciences
590
A113
Yes (verified by ORBi)
International
0004-6361
1432-0746
Les Ulis
France
[en] stars: early-type ; stars: Wolf-Rayet ; stars: winds ; outflows ; X-rays: stars ; stars: individual: WR 21a
[en] Our dedicated XMM-Newton monitoring, as well as archival Chandra and Swift datasets, were used to examine the behaviour of the WN5h+O3V binary WR 21a at high energies. For most of the orbit, the X-ray emission exhibits few variations. However, an increase in strength of the emission is seen before periastron, following a 1 /D relative trend, where D is the separation between both components. This increase is rapidly followed by a decline due to strong absorption as the Wolf-Rayet (WR) comes in front. The fitted local absorption value appears to be coherent with a mass-loss rate of about 1 × 10[SUP]-5[/SUP] M[SUB]⊙[/SUB] yr[SUP]-1[/SUP] for the WR component. However, absorption is not the only parameter affecting the X-ray emission at periastron as even the hard X-ray emission decreases, suggesting a possible collapse of the colliding wind region near to or onto the photosphere of the companion just before or at periastron. An eclipse may appear as another potential scenario, but it would be in apparent contradiction with several lines of evidence, notably the width of the dip in the X-ray light curve and the absence of variations in the UV light curve. Afterwards, the emission slowly recovers, with a strong hysteresis effect. The observed behaviour is compatible with predictions from general wind-wind collision models although the absorption increase is too shallow. Based on observations collected at ESO as well as with Swift, Chandra, and the ESA science mission XMM-Newton, an ESA Science Mission with instruments and contributions directly funded by ESA Member States and the USA (NASA).
Researchers ; Professionals
http://hdl.handle.net/2268/197849
10.1051/0004-6361/201527051
http://adsabs.harvard.edu/abs/2016A%26A...590A.113G

File(s) associated to this reference

Fulltext file(s):

FileCommentaryVersionSizeAccess
Open access
WR21a_edpsciences.pdfPublisher postprint1.14 MBView/Open

Bookmark and Share SFX Query

All documents in ORBi are protected by a user license.