A dataset provided by the European Space Agency

Proposal ID 014543
Title Companion star reflection during the low-state of Hercules X-1
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DOI https://doi.org/10.5270/esa-cx9u4u9
Principal Investigator, PI Dr Martin Still
Abstract Compton reflection is an important contributor to the energy budgets of AGN andblack hole binaries. However characterizing and quantifying reflection isdifficult because it is dominated by the central source of X-rays. RXTEobservations of the X-ray binary Her X-1 have revealed a light curve consistentwith reflection from the inner facing hemisphere of the companion star duringthe source.s X-ray low-state (the result of obscuration by an edge-on accretiondisk). We request an XMM-Newton observation to confirm this reflection usingspectral diagnostics. Stellar masses, binary size, geometry, temperarture,density, composition and the central irradiating spectrum are well-known. Thismakes Her X-1 a potential calibrator of reflection physics.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-02-09T02:12:20Z/2004-02-23T05:14:35Z
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 2005-04-25T00:00:00Z
Keywords "blackhole binary", "energy budgets", "xray low", "XMM-Newton", "spectral diagnostics", "hercules x", "reflection physics", "central irradiating spectrum", "central source", "xmm newton", "companion star", "compton reflection", "stellar masses", "accretion disk", "companion star reflection", "light curve", "XMM", "binary size", "inner facing hemisphere", "xray binary", "quantifying reflection"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Martin Still, 2005, 'Companion star reflection during the low-state of Hercules X-1', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-cx9u4u9