XMM-Newton X-ray and optical observations of the globular clusters M 55 and NGC 3201-Reference-Cited by-同舟云学术

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XMM-Newton X-ray and optical observations of the globular clusters M 55 and NGC 3201

Published:2005-12-13 Issue:1 Volume:445 Page:155-165
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Webb N. A.,Wheatley P. J.,Barret D.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20053010/pdf

Reference63 articles.

1. The complete set ofASCAX-ray observations of non-magnetic cataclysmic variables

2. Blackburn, J. K. 1995, in Astronomical Data Analysis Software and Systems IV, ed. R. A. Shaw, H. E. Payne, & J. J. E. Hayes (San Francisco: ASP), ASP Conf. Ser., 77, 367

3. The Evolution of the High‐Energy Tail in the Quiescent Spectrum of the Soft X‐Ray Transient Aquila X‐1

4. Tidal heating of globular clusters

5. The faint X-ray sources in and out of omega Centauri: X-ray observations and optical identifications

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1. Accreting White Dwarfs;Handbook of X-ray and Gamma-ray Astrophysics;2024

2. Accreting White Dwarfs;Handbook of X-ray and Gamma-ray Astrophysics;2022

3. The X-ray emissivity of low-density stellar populations;Monthly Notices of the Royal Astronomical Society;2020-01-24

4. A detached stellar-mass black hole candidate in the globular cluster NGC 3201;Monthly Notices of the Royal Astronomical Society: Letters;2018-01-15

5. A Proper Motions Study of the Globular Cluster NGC 3201;The Astronomical Journal;2017-02-27

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