Optical structure of the X-ray globular cluster NGC 6624-Reference-Cited by-同舟云学术

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Optical structure of the X-ray globular cluster NGC 6624

Published:1976-03 Issue: Volume:204 Page:L83
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Bahcall N. A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 48 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Evidence for an intermediate-mass black hole in the globular cluster NGC 6624;Monthly Notices of the Royal Astronomical Society;2017-02-28

2. THE PUZZLING NEGATIVE ORBIT-PERIOD DERIVATIVE OF THE LOW-MASS X-RAY BINARY 4U 1820-30 IN NGC 6624;The Astrophysical Journal;2014-10-21

3. Catalogue of Galactic globular-cluster surface-brightness profiles;The Astronomical Journal;1995-01

4. Evolving, dynamical models for collapsed-core globular clusters - M15 and NGC 6624;The Astrophysical Journal;1992-06

5. Mass-to-light ratios for globular clusters. I - The centrally concentrated clusters NGC 6624, M28 (NGC 6626), and M70 (NGC 6681);The Astronomical Journal;1989-08

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