A dataset provided by the European Space Agency

Proposal ID 065408
Title Probing the High Luminosity End of Elliptical Galaxy X-ray Scaling Relations
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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
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
Last Update 2025-01-27
Keywords "useful tool", "elliptical galaxy", "scaling relations", "lensing systems", "xmm newton", "XMM-Newton", "wide range", "type galaxy", "optical luminosities", "XMM", "hot gas", "530 km", "luminous 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