A dataset provided by the European Space Agency

Name 010886
Title Poor Groups Of Galaxies With Extended X-ray Emission
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108860101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108860301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108860401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108860501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108860601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108860701

DOI https://doi.org/10.5270/esa-qsuwsp9
Author European Space Agency
Description GT- Most galaxies belong to poor groups, and much of the baryonic matter in
collapsed objects in the universe resides in the X-ray emitting intragroup
medium. The distribution, and thermal and chemical properties of this hot gas
provides an ideal laboratory for testing theories of cD galaxy formation and the
effects of star-formation-driven feedback on intergalactic matter. We propose to
observed three very poor groups with extended X-ray emission peaked on a central
bright elliptical galaxy in order to measure the profiles of temperature and
abundances of various elements, and decompose these into components associated
with the central galaxy and the group as a whole.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-12-24T14:54:03Z/2002-07-08T00:10:19Z
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 2003-09-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003, Poor Groups Of Galaxies With Extended X-Ray Emission, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qsuwsp9