A dataset provided by the European Space Agency

Name 014845
Title Further observations of large core globular clusters with XMM_Newton
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148450101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148450701

DOI 10.5270/esa-lepbbc2
Author Dr Didier Barret
Description Globular Clusters (GCs) are known to contain two classes of X-ray sources: the bright sources which are neutron star Low-mass X-ray Binaries (LMXBs); and the dim sources whose nature is still discussed. It has been proposed that they could be: cataclysmic variables; X-ray transients in quiescence; or millisecond pulsars, where indeed all these objects have recently been found in the central region of the GC 47 Tuc. We propose to continue our investigations of GCs with large cores, to include five more GCs, and use the XMM-Newton spectral capabilities to determine the nature of their dim X-ray sources. Characterizing the content of GCs is of considerable interest for theories of binary production and evolution, as well as dynamical evolution and survival of GCs.
Publication XMM-Newton X-ray and optical observations of the globular clusters M 55 and NGC 3201 . Webb, N. A., Wheatley, P. J., . A&A . 445-155 . 2006 . 2006A&A...445..155W ,
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 ,
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 ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
XMM-Newton observations of faint X-ray sources in globular clusters . Webb, N. A., Barret, D., . AdSpR . 38-2930 . 2006 . 2006AdSpR..38.2930W ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, D...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-05-25T08:37:50Z/2003-07-06T22:11:50Z
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 2004-09-07T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-09-07T00:00:00Z, 014845, 17.56_20190403_1200. https://doi.org/10.5270/esa-lepbbc2