A dataset provided by the European Space Agency

Name 020045
Title CYG OB2: 3 NON-THERMAL RADIO EMITTERS AND A YOUNG GLOBULAR CLUSTER IN ONE SHOT
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200450201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200450301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200450401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200450501

DOI https://doi.org/10.5270/esa-u5wi2pn
Author Dr GREGOR RAUW
Description We propose to observe the core of the extremely young cluster Cyg OB2. This
cluster contains 3 very massive X-ray bright O-type stars known to display a
variable non-thermal radio emission. By simultaneously monitoring these stars
with XMM, the VLA and optical spectroscopy, and by combining these data with
forthcoming INTEGRAL data we will be able to obtain unprecedented information
on the still mysterious origin of relativistic particles in the stellar winds
of early- type stars. The requested XMM observations will further provide the
deepest yet X-ray survey of this region which is believed to harbour a very
young globular cluster containing more than 100 O-stars therefore providing
information on the earliest phases of star formation in high-density clusters.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-10-29T23:16:45Z/2004-11-29T03:18:52Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2005-12-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr GREGOR RAUW, 2005, 020045, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-u5wi2pn