A dataset provided by the European Space Agency

Name 011227
Title Element Abundances in Galaxy Groups
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112270301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112270501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112270601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112270701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112271001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112271101

DOI https://doi.org/10.5270/esa-53u8qvx
Author European Space Agency
Description GT- Metals injected into the hot gas in galaxy groups preserve a record
of the history of chemical evolution and gas ejection for their
constituent galaxies. The ratio of Fe to alpha elements as a function
of radius will constrain the history of SNI and SNII activity, and
emission from individual group galaxies will constrain the stripping
of gas and dark halos. We have selected a sample consisting of the two
most X-ray luminous Hickson compact groups, and a loose group of
comparable X-ray brightness. Comparison between these systems will
clarify the nature of compact groups and the dynamical evolution of
all groups.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-12-09T14:19:07Z/2003-06-30T04:02:11Z
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 2004-07-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004, Element Abundances In Galaxy Groups, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-53u8qvx