VARIABLE O VI AND N V EMISSION FROM THE X-RAY BINARY LMC X-3: HEATING OF THE BLACK HOLE COMPANION-Reference-Cited by-同舟云学术

VARIABLE O VI AND N V EMISSION FROM THE X-RAY BINARY LMC X-3: HEATING OF THE BLACK HOLE COMPANION

Published:2010-08-09 Issue:3 Volume:140 Page:794-803
ISSN:0004-6256
Container-title:The Astronomical Journal
language:
Short-container-title:The Astronomical Journal

Author:

Song Limin,Tripp Todd M.,Wang Q. Daniel,Yao Yangsen,Cui Wei,Xue Yongquan,Orosz Jerome A.,Steeghs Danny,Steiner James F.,Torres Manuel A. P.,McClintock Jeffrey E.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference26 articles.

1. MIKE: A Double Echelle Spectrograph for the Magellan Telescopes at Las Campanas Observatory

2. FUSEObservations of a Full Orbit of Hercules X‐1: Signatures of Disk, Star, and Wind

3. Discovery of a massive unseen star in LMC X-3

4. Ultraviolet observations of accretion disk in LMC X-3

5. AChandraSpectroscopic Survey of Persistent Black Hole Candidates

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2. THE MASS OF THE BLACK HOLE IN LMC X-3;The Astrophysical Journal;2014-10-06

3. MODELING THE OPTICAL-X-RAY ACCRETION LAG IN LMC X-3: INSIGHTS INTO BLACK-HOLE ACCRETION PHYSICS;The Astrophysical Journal;2014-02-20

4. Mass Measurements of Stellar and Intermediate-Mass Black Holes;Space Science Reviews;2013-12-10

5. XMM–Newton/Reflection Grating Spectrometer detection of the missing interstellar O vii Kα absorption line in the spectrum of Cyg X-2;Monthly Notices of the Royal Astronomical Society;2013-02-23