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A metal deficient early B-type star near the edge of the galactic disk

Research output: Contribution to journal › Article › peer-review

Abstract

High resolution spectra of an early B-type star associated with the H II region detected by de Geus et al. (1993) are analysed using LTE model atmosphere techniques to derive stellar atmospheric parameters and a chemical composition. A distance to the star of 8.2 kpc is estimated, placing it near the edge of the galactic disk and closer than the kinematic distance of 20 kpc to the H II region, calculated by de Geus et al. A differential line by line abundance analysis with respect to the spectroscopic standard tau Sco indicates a significant metal depletion, with elements down on average by -0.5 dex.
Original languageEnglish
Pages (from-to)164-170
Number of pages7
JournalAstronomy and Astrophysics
Volume305
Publication statusPublished - 1996

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