Black Hole Systems Seen at High Spectral Resolution: Inflow and Outflow

Details Black Hole Systems Seen at High Spectral Resolution: Inflow and Outflow Black Hole Systems Seen at High Spectral Resolution: Inflow and Outflow

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.300...67l&link_type=abstract

Astrophysics and Space Science, Volume 300, Issue 1-3, pp. 67-70

Astronomy and Astrophysics

Astrophysics

2

Galaxies, Active, Quasars, General, X-Ray, Black Holes, Binary, Micro-Quasars, Individual Mcg&Minus, 6-30-15, Iras 18325-5926, Grs 1915+105

Scientific paper

High-resolution Chandra and XMM-Newton X-ray spectroscopic studies of stellar and supermassive black holes have revealed that these phenomenologically different systems share many common physical characteristics. The observed outflows in the micro-quasar GRS 1915+105, the Seyfert 1 galaxy MCG 6-30-15 and the Seyfert 2 galaxy IRAS 18325-5926 are the focus of this proceeding.

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