Addendum: X-Ray Sources and Their Optical Counterparts in the Globular Cluster M4 (vol. 609, pg 755 [2004])

Authors
  • C. Bassa
  • D. Pooley
  • L. Homer
  • F. Verbunt
  • B.M. Gaensler
  • W.H.G. Lewin
  • S.F. Anderson
  • B. Margon
  • V.M. Kaspi
  • M. van der Klis
Publication date 2005
Journal Astrophysical Journal
Volume | Issue number 619
Pages (from-to) 1189-1189
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract Luigi Bedin and Ivan King have informed us that the X-ray source CX 2 is in fact the candidate quasi-stellar object (QSO) identified by L.-R. Bedin et al. (<A href="bib_query?2004ApJ...609..755B">ApJ, 609, 755 [2004]</A>). The figure below shows a finding chart of the area around the X-ray position of CX 2 and allows for a direct comparison with the finding chart (Fig. 5) of Bedin et al. (2003).
Document type Article
Related publication X-ray sources and their optical counterparts in the globular cluster M4
Published at https://doi.org/10.1086/426683
Published at http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJ...619.1189B&db_key=AST&high=3ed1d2904207040
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