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New Distances to the Magellanic Clouds
Published online by Cambridge University Press: 12 April 2016
Abstract
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The mean phase magnitudes at the IV waveband (1.05 micron) of thirteen Cepheids in the SMC and the LMC and nine Cepheids in groups and clusters in the Galaxy, are used in conjunction with periods, to construct P–L(IV) relations in these galaxies. The slopes and the dispersions of the relations are nearly the same. We derive a distance modulus of 19.11±0.07 for the SMC and 18.82±0.07 for the LMC.
- Type
- Part III. Extragalactic Cepheids and the PL Relation
- Information
- International Astronomical Union Colloquium , Volume 82: Cepheids: Theory and Observations , 1985 , pp. 223 - 224
- Copyright
- Copyright © Cambridge University Press 1985
References
de Vaucouleurs, G. (1978). The extragalactic distance scale II. Distances of the nearest galaxies from primary indicators, Ap. J.
223, pp. 730–739.10.1086/156306CrossRefGoogle Scholar
Fernie, J. D. & McGonegal, R. (1983). Cepheids in open clusters and associations, Ap.J., 275, pp. 732–736.10.1086/161570CrossRefGoogle Scholar
Gascoigne, S. C.B. (1974). Metal abundance and the luminosities of Cepheids, Mon. Not. R. astr. Soc., 166, Short comm. pp. 25–27.10.1093/mnras/166.1.25PCrossRefGoogle Scholar
McAlary, C. W., Madore, B. F., McGonegal, R.
McLaren, R. A., & Welch, D. L. (1983). The distance to NGC 6822 from infrared photometry of Cepheids, Ap.J.
273, pp. 539–542.Google Scholar
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