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...
Main Authors: | Homan, Jeroen, Neilsen, Joseph M. G. |
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Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2015
|
Online Access: | http://hdl.handle.net/1721.1/95457 |
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