Published 1993
| Published
Book Section - Chapter
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Baade-Wesselink Distances to MS and M92
- Creators
-
Cohen, J. G.
- Others:
- Smith, Graeme H.
- Brodie, Jean P.
Chicago
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Abstract
A Baade-Wesselink analysis has been performed using new optical and infrared photometry of four RR Lyrae variables in the globular cluster M5 and two in M92. We obtain a distance to M5 of 6.9 ± 0.45 kpc and to M92 of 7.85 ± 0.45 kpc, with a 0.3 kpc additional systematic uncertainty. These results are in excellent agreement with the previously published distances, based on matching the globular cluster main sequence to that defined by the field subdwarfs of known distance.
Additional Information
© 1993 Astronomical Society of the Pacific. Provided by the NASA Astrophysics Data System. I thank Keith Matthews, who collaborated in the infrared observing.Attached Files
Published - 1993ASPC___48___78C.pdf
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1993ASPC___48___78C.pdf
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Additional details
- Eprint ID
- 96250
- Resolver ID
- CaltechAUTHORS:20190610-134324219
- Created
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2019-06-10Created from EPrint's datestamp field
- Updated
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2019-10-03Created from EPrint's last_modified field
- Series Name
- Astronomical Society of the Pacific Conference Series
- Series Volume or Issue Number
- 48