Proposal ID | 065408 |
Title | Probing the High Luminosity End of Elliptical Galaxy X-ray Scaling Relations |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654080301 |
DOI | https://doi.org/10.5270/esa-k0w7sq7 |
Principal Investigator, PI | Prof Jimmy Irwin |
Abstract | Scaling relations between L_X, L_opt, T_X, and sigma for elliptical galaxies area useful tool to probe the hydrodynamical state of hot gas within early-typegalaxies. The comparison of these relations to those of groups and clusters alsoprovides insight into the self-similarity behavior of hot gas over a wide rangeof potential well depths. We propose XMM-Newton observations of eight of themost massive and luminous galaxies discovered in the Sloan Digital Sky Survey toextend these relations for elliptical galaxies to optical luminosities a factorof three more luminous than in previous studies. Two of the galaxies are lensesin spectacular strong lensing systems, including a galaxy with an astoundingstellar velocity dispersion of 530 km/s. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2010-12-07T16:56:09Z/2010-12-26T00:31:39Z |
Version | 17.56_20190403_1200 |
Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2012-01-29T00:00:00Z |
Keywords | "optical luminosities", "luminous galaxy", "wide range", "XMM", "530 km", "type galaxy", "xmm newton", "useful tool", "hot gas", "scaling relations", "XMM-Newton", "lensing systems", "elliptical galaxy" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Prof Jimmy Irwin, 2012, 'Probing the High Luminosity End of Elliptical Galaxy X-ray Scaling Relations', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-k0w7sq7 |