COMPARISON OF THE OPEN CLUSTER AND SURFACE BRIGHTNESS DISTANCE SCALESFOR GALACTIC CLASSICAL CEPHEIDS

Citation
P. Fouque et Wp. Gieren, COMPARISON OF THE OPEN CLUSTER AND SURFACE BRIGHTNESS DISTANCE SCALESFOR GALACTIC CLASSICAL CEPHEIDS, Astrophysical letters & communications, 31(1-6), 1995, pp. 243-250
Citations number
17
Categorie Soggetti
Astronomy & Astrophysics
ISSN journal
08886512
Volume
31
Issue
1-6
Year of publication
1995
Pages
243 - 250
Database
ISI
SICI code
0888-6512(1995)31:1-6<243:COTOCA>2.0.ZU;2-4
Abstract
We compare a new period-luminosity (PL) relation, derived by the ZAMS- fitting method for 32 cluster and association Cepheids, to the best de termined Baade-Wesselink (BW) PL relation for 100 stars. Eighteen star s in common lead to conclude that BW and ZAMS-fitting distances can ag ree within 0.1 mag, after proper allowance of possible systematic effe cts.