Low-mass X-ray binaries as a stellar mass indicator for the host galaxy
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- 21 March 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 349 (1) , 146-168
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This publication has 40 references indexed in Scilit:
- ChandraObservation of Low‐Mass X‐Ray Binaries in the Elliptical Galaxy M84The Astrophysical Journal, 2002
- X-Ray Probes of Cosmic Star Formation HistoryThe Astrophysical Journal, 2001
- Diffuse Gas and Low‐Mass X‐Ray Binaries in theChandraObservation of the S0 Galaxy NGC 1553The Astrophysical Journal, 2001
- Stellar Mass‐to‐Light Ratios and the Tully‐Fisher RelationThe Astrophysical Journal, 2001
- The Mass Assembly and Star Formation Characteristics of Field Galaxies of Known MorphologyThe Astrophysical Journal, 2000
- Correcting for the Effects of Interstellar ExtinctionPublications of the Astronomical Society of the Pacific, 1999
- X-ray properties of bright far-infrared galaxiesThe Astrophysical Journal, 1992
- Globular clusters in the interacting galaxies NGC 1549 and NGC 1553The Astronomical Journal, 1990
- Confidence limits for small numbers of events in astrophysical dataThe Astrophysical Journal, 1986
- Contributions to galaxy photometry. II - Standard total magnitudes and colors of bright galaxies from multiaperture photoelectric photometry in the UBV systemThe Astrophysical Journal Supplement Series, 1977