A&A 442, 159-163 (2005)
DOI: 10.1051/0004-6361:20053357
The standard candle aspect of carbon stars
P. Battinelli1 and S. Demers21 INAF, Osservatorio Astronomico di Roma, Viale del Parco Mellini 84, 00136 Roma, Italia
e-mail: battinel@oarhp1.rm.astro.it
2 Département de Physique, Université de Montréal, CP 6128, succursale centre-ville, Montréal, Québec H3C 3J7, Canada
e-mail: demers@astro.umontreal.ca
(Received 3 May 2005 / Accepted 3 July 2005 )
Abstract
This paper represents the second part of our effort to summarise
various aspects of our homogeneous survey of carbon stars in nearby galaxies.
Here we investigate the relationships between the size of the C star populations
and the luminosity of the parent galaxies. We also
explore the constancy of
for various metallicities
and properties of the parent galaxies. We conclude that C stars are a viable
standard candle for galaxies large enough to contain one hundred or more C stars.
The application of narrow-band filters limits, however, the use of C stars
as standard candles to no more than ~2 Mpc with currently available
ground-based telescopes. Near-IR photometry from space observations can
significantly push the limit of detectability of C stars thus making them an
interesting alternative to the TRGB method.
Key words: stars: carbon -- stars: AGB and post-AGB -- cosmology: distance scale
SIMBAD Objects
© ESO 2005

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