Theoretical zero age main sequences revisited

Citation
V. Castellani et al., Theoretical zero age main sequences revisited, ASTRON ASTR, 349(3), 1999, pp. 834-838
Citations number
20
Categorie Soggetti
Space Sciences
Journal title
ASTRONOMY AND ASTROPHYSICS
ISSN journal
00046361 → ACNP
Volume
349
Issue
3
Year of publication
1999
Pages
834 - 838
Database
ISI
SICI code
0004-6361(199909)349:3<834:TZAMSR>2.0.ZU;2-M
Abstract
Zero Age Main Sequence (ZAMS) models with updated physical inputs are prese nted for selected assumptions about the chemical composition, covering the ranges 0.6 < M < 1.2 M., 0.0001 < Z < 0.04, 0.23 < Y < 0.34. The HR diagram location of the ZAMS as a function of Y and Z is discussed both in the the oretical (logL, logT(eff)) and in the observational (M-upsilon, B-V) diagra ms, showing that the V magnitude presents an increased dependence on Z to b e taken into account when discussing observational evidences. Analytical re lations quantifying both these dependences are derived. Implications for th e galactic helium to heavier elements enrichment Delta Y/Delta Z are finall y discussed.