Based in part on observations made with the European Southern Observatory (ESO) telescopes obtained from the ESO/ST-ECF Science Archive Facility.
The influence of the C+N+O abundances on the determination of the relative ages of globular clusters: the case of NGC 1851 and NGC 6121 (M4)
Article first published online: 14 SEP 2009
© 2009 The Authors. Journal compilation © 2009 RAS
Monthly Notices of the Royal Astronomical Society: Letters
Volume 399, Issue 1, pages L151–L155, October 2009
How to Cite
D'Antona, F., Stetson, P. B., Ventura, P., Milone, A. P., Piotto, G. and Caloi, V. (2009), The influence of the C+N+O abundances on the determination of the relative ages of globular clusters: the case of NGC 1851 and NGC 6121 (M4). Monthly Notices of the Royal Astronomical Society: Letters, 399: L151–L155. doi: 10.1111/j.1745-3933.2009.00756.x
This paper makes use of data obtained from the Isaac Newton Group Archive which is maintained as part of the CASU Astronomical Data Centre at the Institute of Astronomy, Cambridge.
- Issue published online: 1 OCT 2009
- Article first published online: 14 SEP 2009
- Accepted 2009 August 11. Received 2009 July 31; in original form 2009 June 27
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