A dataset provided by the European Space Agency

Proposal ID 011246
Title Black hole soft X-ray transients in quiescence SSC_11
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DOI https://doi.org/10.5270/esa-zm9ri10
Principal Investigator, PI Dr Michael Watson
Abstract GT-The defining property of a black hole is its event horizon through whichmatter and energy can rain in, but from which nothing can escape. Proof ofthe existence of event horizons is a foremost goal of astrophysics. However,the goal is an extraordinary challenge since no photon can reach us from thehorizon. We propose to establish the reality of event horizons bycomparing in quiescent X-ray novae the behaviour of accreting black holes tothe behaviour of accreting neutron stars. A by-product of this study will bea handle on the processes that transport angular momentum in accretion discs.Guided by earlier work and a new paradigm for accretion - the ADAFmodel - we propose to observe A0620-00 and GRO J1655-40.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-08-29T23:34:13Z/2002-03-19T02:27:30Z
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 2004-09-17T00:00:00Z
Last Update 2025-01-27
Keywords "event horizon", "defining property", "a0620 00", "accretion discs", "quiescence ssc_11", "accreting blackhole", "transport angular momentum", "quiescent xray novae", "accreting neutron stars", "adaf model", "gro j1655", "event horizons"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Michael Watson, 2004, 'Black hole soft X-ray transients in quiescence SSC_11', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zm9ri10