Metal abundance and helium content of the open cluster NGC 7789: Evidence for mass loss
- 1 November 1979
- journal article
- research article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 66 (1) , 201-209
- https://doi.org/10.1007/bf00648371
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- Cyanogen strengths and ultraviolet excesses of evolved stars in 17 globular clusters from DDO photometry.The Astrophysical Journal Supplement Series, 1977
- DDO and UBV photometry of NGC 7789.The Astronomical Journal, 1977
- The Chemical Evolution of the Galactic HaloThe Astrophysical Journal, 1976
- The Horizontal Branch and the Cosmic Abundance of HeliumMonthly Notices of the Royal Astronomical Society, 1973
- The abnormally metal-rich globular NGC 6352The Astrophysical Journal, 1972
- Red Giants in old Open ClustersMonthly Notices of the Royal Astronomical Society, 1970
- ON the Interpretation of the Color-Magnitude Diagrams of M67 and NGC 188The Astrophysical Journal, 1969
- Stellar Evolution Within and Off the Main SequenceAnnual Review of Astronomy and Astrophysics, 1967
- Intermediate-Age Star Clusters.The Astrophysical Journal, 1962
- The Color-Magnitude Diagram for the Galactic NGC 7789.The Astrophysical Journal, 1958