Pulsational MV versus [Fe/H] relation(s) for globular cluster RR Lyrae variables
暂无分享,去创建一个
V. Ripepi | V. Ripepi | M. Marconi | V. Castellani | M. Marconi | F. Caputo | V. Castellani | F. Caputo
[1] Garching,et al. Hubble Space Telescope Observations of the Large Magellanic Cloud Field around SN 1987A: Distance Determination with Red Clump and Tip of the Red Giant Branch Stars , 1999, astro-ph/9910082.
[2] R. Stellingwerf,et al. Convection in pulsating stars. III - The RR Lyrae instability strip , 1984 .
[3] Michael J. West,et al. The globular cluster system of the Galaxy. III: measurements of radial velocity and metallicity for 60 clusters and a compilation of metallicities for 121 clusters , 1984 .
[4] A. Walker,et al. CCD Photometry of Galactic Globular Clusters.III.IC 4499 , 1996 .
[5] Forrest J. Rogers,et al. Updated Opal Opacities , 1996 .
[6] V. Castellani,et al. The evolution of He-burning stars - Horizontal and asymptotic branches in Galactic globulars , 1991 .
[7] M. Mateo,et al. B,V photometry of the RR Lyrae stars in the very metal-poor globular cluster NGC 5053 , 1995 .
[8] A. Walker. BVI CCD Photometry of Galactic Globular Clusters. II. M68 , 1994 .
[9] R. J. Dickens,et al. Photographic photometry of RR Lyrae variables in the globular cluster M15 , 1984 .
[10] Two-Color CCD Photometry of Variable Stars in NGC 7006 , 1999 .
[11] Robert F. Stellingwerf,et al. Pulsation and stability of RR Lyrae stars. 1: Instability strip , 1994 .
[12] Mario G. Lattanzi,et al. Ages of globular clusters from hipparcos parallaxes of local subdwarfs , 1997 .
[13] B. Carney,et al. The slope of the RR Lyrae MV−[Fe/H] relation , 1998 .
[14] J. S. Wright,et al. Discovery of an "alpha" Element-Poor Halo Star in a Search for Very Low- Metallicity Disk Stars , 1997 .
[15] R. Christy,et al. A study of pulsation in RR Lyrae models. , 1966 .
[16] A. Weiss,et al. An updated theoretical scenario for globular cluster stars , 1997, astro-ph/9707180.
[17] A. Heck,et al. Post-Hipparcos cosmic candles , 1999 .
[18] Daniel Egret,et al. Harmonizing Cosmic Distance Scales in a Post‐Hipparcos Era , 1999 .
[19] T. S. van Albada,et al. On the Two Oosterhoff Groups of Globular Clusters , 1973 .
[20] R. Zinn,et al. The Metallicity Dependence of RR Lyrae Absolute Magnitudes from Synthetic Horizontal-Branch Models , 1999, astro-ph/9912226.
[21] THE GIANT, HORIZONTAL, AND ASYMPTOTIC BRANCHES OF GALACTIC GLOBULAR CLUSTERS. I. THE CATALOG, PHOTOMETRIC OBSERVABLES, AND FEATURES , 1999, astro-ph/9906248.
[22] G. A. Rutledge,et al. GALACTIC GLOBULAR CLUSTER METALLICITY SCALE FROM THE CA II TRIPLET II. RANKINGS, COMPARISONS, AND PUZZLES , 1997, astro-ph/9707068.
[23] G. Bono,et al. Nonlinear investigation of the pulsational properties of RR Lyrae variables , 1997 .
[24] A. Sandage. Globular cluster ages determined from the Oosterhoff period−metallicity effect using oxygen-enhanced isochrones. III , 1993 .
[25] William E. Harris,et al. A Catalog of Parameters for Globular Clusters in the Milky Way , 1996 .
[26] Filippina Caputo,et al. The period-magnitude diagram of RR Lyrae stars — I. The controversy about the distance scale , 1997 .
[27] Soo-Chang Rey,et al. CCD Photometry of the Globular Cluster ω Centauri. I. Metallicity of RR Lyrae Stars from Caby Photometry , 2000 .
[28] R. G. Gratton,et al. Abundances for globular cluster giants: I. homogeneous metallicities for 24 clusters , 1996, astro-ph/9607078.
[29] I. Shelton,et al. New CCD Observations of the RR Lyrae Variables in the Oosterhoff Type IICluster M9 , 1999 .
[30] M. Marconi,et al. Metal-rich RR Lyrae Variables. II. The Pulsational Scenario , 1997, astro-ph/9702083.
[31] I. Pérez-Fournon,et al. Globular clusters : X Canary Islands Winter School of Astrophysics , 1999 .
[32] Oscar Straniero,et al. The alpha -enhanced Isochrones and Their Impact on the FITS to the Galactic Globular Cluster System , 1993 .
[33] A. Weiss,et al. GALACTIC GLOBULAR CLUSTER STARS : FROM THEORY TO OBSERVATION , 1998, astro-ph/9811329.
[34] D. Mcnamara. The Slope of the RR Lyrae Variables \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT , 1999 .
[35] S. Demers,et al. Variable stars of NGC 4833. , 1977 .
[36] Young-Wook Lee. Stellar evolution and period changes in RR Lyrae stars , 1991 .
[37] R. Stellingwerf. Modal stability of RR Lyrae stars. , 1975 .
[38] RR Lyrae Variables in the Globular Cluster M55. The First Evidence for Nonradial Pulsations in RR Lyrae Stars , 1998, astro-ph/9812302.
[39] R. Zinn,et al. The horizontal-branch stars in globular clusters. I - The period-shift effect, the luminosity of the horizontal branch, and the age-metallicity relation , 1990 .
[40] V. Ripepi,et al. RR Lyrae variables in M5 as a test of pulsational theory , 1999, astro-ph/9902279.
[41] A. N. Cox. Masses of RRd Variables Using Livermore OPAL Opacities , 1991 .
[42] Alistair R. Walker,et al. CCD Photometry of Galactic Globular Clusters. IV. The NGC 1851 RR Lyrae Variables , 1998, astro-ph/9804339.
[43] Gisella Clementini,et al. Distances, Ages, and Epoch of Formation of Globular Clusters , 1999, astro-ph/9902086.
[44] Santi Cassisi,et al. Metal-rich RR Lyrae Variables. I. The Evolutionary Scenario , 1996, astro-ph/9609153.