Computer Science
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..73862115f&link_type=abstract
VizieR On-line Data Catalog: J/MNRAS/386/2115. Originally published in: 2008MNRAS.386.2115F
Computer Science
Stars: Variable, Photometry
Scientific paper
Infrared and optical absolute magnitudes are derived for the type II Cepheids kappa Pav and VY Pyx using revised Hipparcos parallaxes and for kappa Pav, V553 Cen and SW Tau from pulsational parallaxes. Revised Hipparcos and HST parallaxes for RR Lyrae agree satisfactorily and are combined in deriving absolute magnitudes. Phase-corrected J, H and Ks mags are given for 142 Hipparcos RR Lyraes based on Two-Micron All-Sky Survey observations. Pulsation and trigonometrical parallaxes for classical Cepheids are compared to establish the best value for the projection factor (p) used in pulsational analyses.
(3 data files).
Feast Michael W.
Kinman Thomas D.
Laney Cliford D.
van Leeuwen Floor
Whitelock Patricia A.
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