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- W2000478449 abstract "view Abstract Citations (14) References (14) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Bright Stars in the Galactic Globular M5 Brocato, E. ; Castellani, V. ; Ripepi, V. Abstract We present a CCD investigation of the galactic globular M5 aimed to increase the statistical relevance of the available sample of evolving bright stars. Previous investigations, limited to the outer cluster region, have been extended toward the cluster center, more than doubling the number of observed luminous stars. On this basis, we discuss a statistically relevant sample, rich of 415 HB stars. The occurrence of a gap in the blue side of the HB is suggested. Comparison to the current evolutionary scenario discloses a good agreement concerning both the C-M diagram location and the relative abundance of stars in the advanced evolutionary phases, supporting our present knowledge of the evolution of low mass stars. Determination of the amount of the original helium content through the ratio R N(HB)/N(RGB) gives $Y = 0.22 pm 0.02$. Publication: The Astronomical Journal Pub Date: April 1995 DOI: 10.1086/117394 arXiv: arXiv:astro-ph/9407022 Bibcode: 1995AJ....109.1670B Keywords: Brightness; Galactic Evolution; Globular Clusters; Horizontal Branch Stars; Milky Way Galaxy; Stellar Evolution; Stellar Luminosity; Abundance; Charge Coupled Devices; Color-Magnitude Diagram; Galactic Structure; Helium; Star Distribution; Astronomy; GLOBULAR CLUSTERS: INDIVIDUAL: M5; STARS: EVOLUTION; Astrophysics E-Print: 16 pages, Standard TeX, 4 figures available upon request from brocato@astrte.te.astro.it full text sources arXiv | ADS | data products SIMBAD (1)" @default.
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- W2000478449 date "1995-04-01" @default.
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- W2000478449 title "Bright stars in the galactic globular M5" @default.
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