The Nature of the Accretion Flow in the Low-hard State

Details The Nature of the Accretion Flow in the Low-hard State The Nature of the Accretion Flow in the Low-hard State

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..191r&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

Astronomical Observations, Black Holes, Galactic Nuclei, Stellar Coronae, X-Ray, Black Holes, Galactic Nuclei, Circumnuclear Matter, And Bulges, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

Observations over the past number of years have cast significant doubt on the current paradigm describing the geometry of the accretion flow in the low-hard state. Here, we summarize the relevant observations in addition to a number of new Suzaku observations and discuss their implications for the geometry of the accretion flow in the low-hard state.

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