A dataset provided by the European Space Agency

Title The X-ray source populations of different stellar generations in the LMC
DOI https://doi.org/10.5270/esa-mrrw78x
Abstract We propose XMM observations of 5 regions of the LMC with well constrained youngstellar populations of ages virgul10-50 Myr.These observations will probe the X-raysource populations in regions of varying stellar content, down to a luminosityof virgul10^33 erg/s in the nearest star-forming galaxy. From the opticalcounterparts of the detected sources we will classify them as supergiants orBe/X-ray binaries (SG- or Be-XRBs, respectively), while based on X-ray spectraand timing analysis we will identify X-ray binary pulsars (XBPs). We will usethese results to investigate the connection between stellar and XRB populations.The proposed observations will complement existing Chandra and XMM observationsof the LMC as well as similar studies of other galaxies where these faint XRB populations cannot be observed.
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-04-30T09:04:10Z/2010-05-06T18:36:42Z
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 2011-05-21T00:00:00Z
Keywords XMM-Newton, OM, RGS, EPIC, X-ray, Multi-Mirror, SAS
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Vallia Antoniou, 2011, 'The X-ray source populations of different stellar generations in the LMC', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mrrw78x