Published July 25, 2005
| Version v1
Journal article
Oxygen in the Blanco 1 open cluster
Creators
- 1. CSPA/SPME, Building 28M, Monash University, VIC 3800 (Australia)
- 2. School of Physics and Chemistry, Keele University, STAFFS, ST5 5BG (United Kingdom)
Description
We present preliminary measurements of the iron and oxygen abundances in 8 F/G-type stars of the young Blanco 1 open cluster. Previous work suggested that this cluster has a high metal content, but a Li-abundance pattern similar to the solar-metallicity Pleiades. This would contradict the strong metallicity dependence predicted by models of pre-main sequence Li depletion. Our new results show that the metallicity of the cluster is lower than previously believed, with [Fe/H] approximately solar and with [O/Fe]∼ 0.1
Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysa.2005.05.048;
- PII
- S0375-9474(05)00689-5;
Publishing Information
- Journal Title
- Nuclear Physics. A
- Journal Volume
- 758
- Journal Page Range
- p. 280-283
- ISSN
- 0375-9474
- CODEN
- NUPABL
Conference
- Title
- 8. international symposium on nuclei in the cosmos
- Dates
- 19-23 Jul 2004
- Place
- Vancouver, BC (Canada)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37042829
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; ELEMENT ABUNDANCE; HYDROGEN; IRON; OXYGEN; STARS
- Descriptors DEC
- ABUNDANCE; ELEMENTS; METALS; NONMETALS; PHYSICS; TRANSITION ELEMENTS
Optional Information
- Copyright
- Copyright (c) 2005 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.