Erratum: ``Some Constraints on the Effect of Age and Metallicity on the Low-Mass X-Ray Binary Formation Rate''

Open Access
Authors
  • A. Kundu
  • T.J. Maccarone
  • S.E. Zepf
  • T.H. Puzia
Publication date 2004
Journal Astrophysical Journal
Volume | Issue number 600
Pages (from-to) L91-L91
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract The number of low-mass X-ray binaries in NGC 4365 that are within 0.5" of a globular cluster and considered to be matches is 18, not 23 as mistakenly reported in the first paragraph of ยง 3. The correct number is used elsewhere in the above Letter. The fraction of low-mass X-ray binaries that are associated with globular clusters in NGC 4365 is indeed 40% as noted later in the same paragraph. We thank W. Lewin for alerting us to this error.
Document type Erratum / Corrigendum
Published at https://doi.org/10.1086/381435
Published at http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJ...600L..91K&db_key=AST&high=41f4b95c5118374
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