Abundance analysis of stars in NGC 6522 (Castro+, 1995)

Details Abundance analysis of stars in NGC 6522 (Castro+, 1995) Abundance analysis of stars in NGC 6522 (Castro+, 1995)

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ycat..41110017c&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/111/17. Originally published in: 1995A&AS..111...17C

Physics

Clusters: Globular, Spectroscopy, Abundances

Scientific paper

The CASPEC echelle spectrograph at the ESO 3.6 m telescope was used to obtain high resolution spectra of Arp 1145 and Arp 2240, two stars of the Baade Window, near the globular cluster NGC 6522. From a detailed analysis using equivalent widths and spectrum synthesis we derive the stellar parameters (Teff, log g and [M/H])=(4750,1.2,-0.9) and (5000,2.15,+0.2), respectively for Arp 1145 and Arp 2240. (1 data file).

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