A dataset provided by the European Space Agency

Name 011292
Title XMM X-ray Spectroscopy of Microquasars During Their X-Ray.. SSC_10
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112920701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112920801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112920901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112921201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112921301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112921401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112921501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112921601

DOI https://doi.org/10.5270/esa-fjy6dhm
Author European Space Agency
Description The galactic superluminal motion sources GRS 1915+105 and GRO J1655-40
are thought to be binary systems containing a stellar-size (7-30 M_sun)
black hole. Yet, they show distinctly different X-ray properties during
their active states than usual black hole transients. We propose to observe
these sources with XMM to search for clues regarding the origin of
relativistic jets, to probe the properties of the compact object, and
to understand the various spectral components and their evolution as
the sources journey through different accretion states. The brightness of
these objects allows only RGS and EPIC PN burst mode observations.
Publication No observations found associated with the current proposal
Instrument EPN, OM, RGS1, RGS2
Temporal Coverage 2003-04-10T13:44:31Z/2005-03-16T20:24:37Z
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 2006-04-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006, Xmm X-Ray Spectroscopy Of Microquasars During Their X-Ray.. Ssc_10, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-fjy6dhm