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
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