A dataset provided by the European Space Agency

Proposal ID 050511
Title A follow-up study of the colliding wind binary Cyg OB2 8a
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505110301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505110401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505110501

DOI https://doi.org/10.5270/esa-byh57pf
Principal Investigator, PI Dr Gregor Rauw
Abstract We propose to observe the colliding wind binary Cyg OB2 #8a (O6If + O5.5III(f))for 3 x 20 ksec near specific orbital phases. Previous XMM-Newton observationsrevealed a modulation of the X-ray flux of this system. At the same time, theradio emission of Cyg OB2 #8a also undergoes a phase-locked variation. The jointanalysis of the variations in the X-ray and radio domains will provideunprecedented information on the interplay between colliding wind interactionsand the acceleration of relativistic particles that produce the non-thermalradio emission. The Cyg OB2 cluster further harbours a number of early-typestars (two of them are non-thermal radio emitters) that are bright X-raysources, as well as a wealth of secondary sources (most of them being low-mass PMS stars).
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-04-29T16:23:01Z/2007-05-03T20:37:49Z
Version 17.56_20190403_1200
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2008-12-11T00:00:00Z
Keywords "specific orbital phases", "colliding wind interactions", "secondary sources", "relativistic particles", "bright xray sources", "phase locked variation", "XMM", "xmm newton", "xray flux", "nonthermal radio emitters", "radio domains", "XMM-Newton", "radio emission", "8a o6if", "nonthermal radio emission", "type stars", "cyg ob2", "cyg ob2 cluster"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Gregor Rauw, 2008, 'A follow-up study of the colliding wind binary Cyg OB2 8a', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-byh57pf