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Table · dataset · 1997

Abundance analysis of stars in NGC 6522

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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.

Description

From a detailed analysis using equivalent widths and spectrum synthesis we derive the stellar parameters (T_eff_, log g and [M/H])=(4750,1.2,-0.9) and (5000,2.15,+0.2), respectively for Arp 1145 and Arp 2240.

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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+as/111/1714 d agoJSON v1
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