A SUPER-EDDINGTON, COMPTON-THICK WIND IN GRO J1655-40?
During its 2005 outburst, GRO J1655-40 was observed at high spectral resolution with the Chandra High-Energy Transmission Grating Spectrometer, revealing a spectrum rich with blueshifted absorption lines indicative of an accretion disk wind-apparently too hot, too dense, and too close to the black h...
| Main Authors: | , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing,
2017-07-12T16:38:07Z.
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| Subjects: | |
| Online Access: | Get fulltext |