A HYBRID MAGNETICALLY/THERMALLY DRIVEN WIND IN THE BLACK HOLE GRO J1655–40?
During its 2005 outburst, GRO J1655-40 was observed twice with the Chandra High Energy Transmission Grating Spectrometer; the second observation revealed a spectrum rich with ionized absorption lines from elements ranging from O to Ni, indicative of an outflow too dense and too ionized to be driven...
Κύριοι συγγραφείς: | Homan, Jeroen, Neilsen, Joseph M. G. |
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Άλλοι συγγραφείς: | MIT Kavli Institute for Astrophysics and Space Research |
Μορφή: | Άρθρο |
Γλώσσα: | en_US |
Έκδοση: |
IOP Publishing
2015
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Διαθέσιμο Online: | http://hdl.handle.net/1721.1/95457 |
Παρόμοια τεκμήρια
Παρόμοια τεκμήρια
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A SUPER-EDDINGTON, COMPTON-THICK WIND IN GRO J1655–40?
ανά: Rahoui, F., κ.ά.
Έκδοση: (2017) -
The quiescent lightcurve and evolutionary state of GRO J1655-40
ανά: Beer, M, κ.ά.
Έκδοση: (2001) -
Echoes from an irradiated disc in GRO J1655-40
ανά: Hynes, R, κ.ά.
Έκδοση: (1998) -
Radiation-hydrodynamic simulations of thermally-driven disc winds in X-ray binaries: A direct comparison to GRO J1655-40
ανά: Higginbottom, N, κ.ά.
Έκδοση: (2018) -
The quiescent light curve and the evolutionary state of GRO J1655-40
ανά: Beer, M, κ.ά.
Έκδοση: (2002)