Eclipsing Broad Emission Lines in Hercules X‐1: Evidence for a Disk Wind?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/549/i=1/a=537/pdf
Reference44 articles.
1. The theory of radiatively driven stellar winds. II - The line acceleration
2. Compton heated winds and coronae above accretion disks. I Dynamics
3. Hydromagnetic flows from accretion discs and the production of radio jets
4. Pulsations and Line Profile Changes in the Ultraviolet Spectrum of Hercules X‐1: Results from a Multiwavelength Campaign
5. Hercules X‐1: Empirical Models of Ultraviolet Emission Lines
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1. FUSEOBSERVATIONS OF A FULL ORBIT OF SCORPIUS X-1;The Astrophysical Journal;2014-09-05
2. FUSEObservations of a Full Orbit of Hercules X‐1: Signatures of Disk, Star, and Wind;The Astrophysical Journal;2007-10
3. Identification of an Extended Accretion Disk Corona in the Hercules X‐1 Low State: Moderate Optical Depth, Precise Density Determination, and Verification of CNO Abundances;The Astrophysical Journal;2005-06
4. The Ultraviolet Spectrum of the Ultracompact X-Ray Binary 4U 1626−67;The Astronomical Journal;2002-12
5. High‐Resolution X‐Ray Spectroscopy of Hercules X‐1 with theXMM‐NewtonReflection Grating Spectrometer: CNO Element Abundance Measurements and Density Diagnostics of a Photoionized Plasma;The Astrophysical Journal;2002-10-10
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