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2008MNRAS.386..313W - Mon. Not. R. Astron. Soc., 386, 313-323 (2008/May-1)
AGB variables and the Mira period-luminosity relation.
WHITELOCK P.A., FEAST M.W. and VAN LEEUWEN F.
Abstract (from CDS):
Carbon-rich stars are also discussed and provide results that are consistent with the above numbers, but with higher uncertainties. Within the uncertainties there is no evidence for a significant difference between the period-luminosity relation zero-points for systems with different metallicity.
Abstract Copyright: ©2008 The Authors. Journal compilation © 2008 RAS
Journal keyword(s): stars: AGB and post-AGB - stars: carbon - stars: oscillations - stars: variables: other
VizieR on-line data: <Available at CDS (J/MNRAS/386/313): stars.dat tablea1.dat tablea3.dat>
Simbad objects: 299
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