A dataset provided by the European Space Agency

Name 040089
Title X-rays from Quiescent Black Holes: Accretion or Jet Powered
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400890101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400890201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400890301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400890401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400890501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400890601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400890701

DOI 10.5270/esa-wp6eozj
Author Prof Wei Cui
Description We propose to obtain X-ray spectra of transient black hole binaries (BHBs) in quiescence. The spectra are expected to provide a severe test of the Compton origin of X-rays from such sources, as expected from accretion-based models. At very low accretion rates, a Comptonized spectrum is expected to appear strongly curved in a log-log plot. However, there is already tentative evidence for the power-law shape of the quiescent X-ray spectrum. If confirmed, it would favor a jet origin of the X-ray emission. However, the quality of existing data is still quite poor. The deep observations proposed here will allow a detailed look at the roles of accretion flows and jets in quiescent BHBs and thus cast light on the issues of accretion-jet coupling and particle acceleration in such systems.
Publication The Galactic plane at faint X-ray fluxes - I. Properties and characteristics of the X-ray source population . Warwick, R. S., Perez-Ramirez, D., . MNRAS . 413-595 . 2011 . 2011MNRAS.413..595W ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Origin of X-ray emission from transient black hole candidates in quiescence . Pszota, Gabor, Zhang, Hui, et all. . MNRAS . 389-423 . 2008 . 2008MNRAS.389..423P ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
The quiescent X-ray spectrum of accreting black holes . Reynolds, Mark T., Reis, Rubens C., et all. . MNRAS . 441-3656 . 2014 . 2014MNRAS.441.3656R ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Tracing the Reverberation Lag in the Hard State of Black Hole X-Ray Binaries . De Marco, B., Ponti, G., et all. . ApJ . 8...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-02-22T15:32:57Z/2007-03-28T03:08:31Z
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 2009-02-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-02-09T00:00:00Z, 040089, 17.56_20190403_1200. https://doi.org/10.5270/esa-wp6eozj