A dataset provided by the European Space Agency

Proposal ID 067372
Title Understanding two new extreme X-ray sources
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673720201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673720301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673720401

DOI https://doi.org/10.5270/esa-tjsbq9x
Principal Investigator, PI Dr Christian Motch
Abstract Our optical identification campaign of hard X-ray sources in the XMM-NewtonGalactic Plane Survey (XGPS) has revealed two exceptional objects. First, sourceXGPS-3 is identified with a heavily absorbed very bright infrared source whichcould be a star as luminous as eta Carina. Second, XGPS-25 has all the featuresexpected from a low-mass X-ray binary whose X-ray emission is strongly shieldedby the accretion disc and if confirmed, would be the first very high inclinationaccretion disc corona known to date. The present proposal aims at obtaining highquality X-ray spectra and time series which will help us to clarify the exactnature of these two objects.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-09-11T04:31:56Z/2012-03-21T16:19:09Z
Version PPS_NOT_AVAILABLE
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 2013-04-10T00:00:00Z
Last Update 2025-01-27
Keywords "quality xray spectra", "eta carina", "heavily absorbed", "XMM-Newton", "bright infrared source", "source xgps", "xray sources", "xray emission", "time series", "XMM", "optical identification campaign", "hard xray sources", "accretion disc"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Christian Motch, 2013, 'Understanding two new extreme X-ray sources', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-tjsbq9x