A dataset provided by the European Space Agency

Name 060201
Title Metal Abundance in Young Elliptical Galaxies
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602010101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602010301

DOI 10.5270/esa-g9cja64
Author Dr Dong-Woo Kim
Description We propose deep XMM-Newton observations of young, post-merger elliptical galaxies. Because their L_X-L_B ratios are low among ellipticals and their stellar populations are significantly metal-enriched, these galaxies are the best candidates to address the biggest unsolved problem of the X-ray study of elliptical galaxies: stellar vs ISM metal abundance discrepancy. Our data, in conjunction with the existing Chandra data will allow us to accurately determine Fe and alpha -elements abundances and to confirm the presence or absence of the relation between L_X-L_B and the metallicity. We will then address various evolutionary scenarios via metal enrichment history.
Publication An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
Investigating the Potential Dilution of the Metal Content of Hot Gas in Early-type Galaxies by Accreted Cold Gas . Su, Yuanyuan, Irwin, Jimmy A., . ApJ . 766-61 . 2013 . 2013ApJ...766...61S ,
Modeling X-Ray Emission around Galaxies . Anderson, Michael E., Bregman, Joel N., . ApJ . 785-67 . 2014 . 2014ApJ...785...67A ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra . Anderson, Michael E., Churazov, Eugene, . MNRAS . 452-3905 . 2015 . 2015MNRAS.452.3905A ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
X-ray-selected broad absorption line quasi-stellar objects . Page, M. J., Carrera, F. J., et all. . MNRAS . 464-4586 . 2017 . 2017MNRAS.464.4586P ,
AGN spectral states from simultane...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-06-23T06:37:52Z/2009-12-24T23:13:29Z
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 2011-01-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-01-27T00:00:00Z, 060201, 17.56_20190403_1200. https://doi.org/10.5270/esa-g9cja64