Name | 011227 |
Title | Element Abundances in Galaxy Groups |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112270301 |
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 |