A dataset provided by the European Space Agency

Name 065032
Title Characterizing the X-ray properties of the earliest magnetic stars
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650320101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650320201

DOI https://doi.org/10.5270/esa-ejw2ejo
Author European Space Agency
Description The recent detection of magnetic fields in massive stars has profoundly changed
our understanding of the structure and evolution of these objects. In addition,
detailed modelling shows that intense magnetic fields can have a strong impact
on the X-ray emission. Currently, only a few tens of magnetic hot stars are
known, and much fewer have been observed at high energies. The observed
diversity of behaviours and the small sample size actually prevent us from
recognizing the overall trends. By doubling the sample size with a small
investment of time, we will be able to undertake such a systematic study of the
X-ray properties of magnetic massive stars, which will help us better understand
which parameters govern their high-energy emission.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-08-30T00:31:18Z/2010-10-16T10:41:38Z
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 2011-11-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011, Characterizing The X-Ray Properties Of The Earliest Magnetic Stars, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ejw2ejo