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Cepheid Distances to Nearby Galaxies

Published online by Cambridge University Press:  12 April 2016

Wolfgang P. Gieren ,
Pablo Candia ,
Pascal Fouqué ,
Gisela Hertling  and
Eduardo Brieva
Wolfgang P. Gieren
Affiliation:
Pontifica Universidad Católica de Chile, Casilla 104, Santiago 22, Chile
Pablo Candia
Affiliation:
Pontifica Universidad Católica de Chile, Casilla 104, Santiago 22, Chile
Pascal Fouqué
Affiliation:
DESPA Observatoire de Paris-Meudon, F-92195 Meudon Cedex France and European Southern Observatory, Casilla 19001, Santiago 19, Chile
Gisela Hertling
Affiliation:
Pontifica Universidad Católica de Chile, Casilla 104, Santiago 22, Chile
Eduardo Brieva
Affiliation:
Observatorio Astronómico Nacional, Apartado Aéreo 2584, Bogotá, Colombia

Abstract

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We have determined new Cepheid distances on a homogeneous system to nine nearby galaxies with Cepheid observations in the V bandpass, using the extensive calibration of the galactic Cepheid PL(V) relation of Gieren, Barnes & Moffett (1993). Absorption corrections to the observed distance moduli were taken from the RC3 catalog (de Vaucouleurs et al. 1991). For most of the galaxies, the galactic PL(V) relation of GBM gives a very good fit to the Cepheid data.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 381 - 382
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

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Gieren, W.P., Barnes, T.G. & Moffett, T.J. 1993, ApJ, 418, 135 CrossRefGoogle Scholar