A dataset provided by the European Space Agency

Name 040353
Title Probing the nature of a very luminous globular cluster X-ray source
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0403530201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0403530301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0403530401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0403530501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0403530601

DOI 10.5270/esa-7slqhr9
Author Dr Albert Kong
Description There are over 400 very luminous (Lx ~ 1e38-1e40 erg-s) globular cluster X-ray sources in nearby galaxies. None are present in our Galaxy, and their nature is unknown. They may be accreting black holes, however, this is quite controversial and it is contrary to theoretical expectations. The distance is too large to make accurate studies of any of them that could reveal their nature. Luckily, there is one such very luminous source, Bo375, in a globular cluster in M31. We propose to perform ten 10 ksec observations of Bo375 and we expect that we will be able to determine the nature of this object.
Publication 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 ,
A Census of the Supersoft X-ray Sources in M31 . Orio, Marina, Nelson, Thomas, et all. . ApJ . 717-739 . 2010 . 2010ApJ...717..739O ,
An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 . Henley, David B., Shelton, Robin L., . ApJS . 187-388 . 2010 . 2010ApJS..187..388H ,
A systematic study of low-mass X-ray binaries in the M31 globular cluster system . Peacock, Mark B., Maccarone, Thomas J., et all. . MNRAS . 407-2611 . 2010 . 2010MNRAS.407.2611P ,
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 ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
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 ,
...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-07-08T23:10:00Z/2006-07-16T10:39:02Z
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 2007-08-12T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-08-12T00:00:00Z, 040353, 17.56_20190403_1200. https://doi.org/10.5270/esa-7slqhr9