A dataset provided by the European Space Agency

Name 020501
Title DO ALL LMXBS FORM WITHIN GLOBULAR CLUSTERS?
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205010101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205010201

DOI 10.5270/esa-8cw6l4w
Author Dr JIMMY IRWIN
Description Recent studies have found that a large fraction of LMXBs within elliptical galaxies reside within globular clusters, prompting claims that all LMXBs are formed within globular clusters. If so, the total X-ray luminosity emanating from LMXBs should scale directly with the globular cluster specific frequency, S_N. Conversely, if there is a significant field-born population of LMXBs this relation will be flatter. We have begun a program to test this claim, but we need to observe galaxies with high values of S_N to confirm our findings. We propose observations of NGC4278 (S_N=8.7) and NGC4526 (S_N=7.7), two nearby gas-poor galaxies with high well-constrained values of S_N. These observations will put stringent constraints on the field-born population of LMXBs in galaxies.
Publication X-ray and multiwavelength view of NGC 4278. A LINER-Seyfert connection? . Younes, G., Porquet, D., et all. . A&A . 517-33 . 2010 . 2010A&A...517A..33Y ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
New constraints on the X-ray spectral properties of type 1 active galactic nuclei . Scott, A. E., Stewart, G. C., et all. . MNRAS . 417-992 . 2011 . 2011MNRAS.417..992S ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
X-ray Emission from Optically Selected Radio-intermediate and Radio-loud Quasars . Miller, B. P., Brandt, W. N., et all. . ApJ . 726-20 . 2011 . 2011ApJ...726...20M ,
A combined optical and X-ray study of unobscured type 1 active galactic nuclei - I. Optical spectra and spectral energy distribution modelling . Jin, Chichuan, Ward, Martin, et all. . MNRAS . 420-1825 . 2012 . 2012MNRAS.420.1825J ,
Study of LINER sources with broad Halpha emission. Spectral energy distribution and multiwavelength correlations . Younes, G., Porquet, D., e...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-05-23T17:13:02Z/2004-06-05T19:14:21Z
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 2005-07-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-07-04T00:00:00Z, 020501, 17.56_20190403_1200. https://doi.org/10.5270/esa-8cw6l4w