Discovery and quantitative spectral analysis of an Ofpe/WN9 (WN11) star in the Sculptor spiral galaxy NGC 300

Abstract

We have discovered an Ofpe/WN9 (WN11 following Smith et al.) star in the Sculptor spiral galaxy NGC 300, the first object of this class found outside the Local Group, during a recent spectroscopic survey of blue supergiant stars obtained at the ESO VLT. The light curve over a five-month period in late 1999 displays a variability at the 0.1 mag level. The intermediate resolution spectra (3800-7200 A) show a very close resemblance to the Galactic LBV AG Car during minimum. We have performed a detailed non-LTE analysis of the stellar spectrum, and have derived a chemical abundance pattern which includes H, He, C, N, O, Al, Si and Fe, in addition to the stellar and wind parameters. The derived stellar properties and the He and N surface enrichments are consistent with those of other Local Group WN11 stars in the literature, suggesting a similar quiescent or post-LBV evolutionary status.

arXiv comment9 pages, 4 figures, 2 tables. Accepted for publication in the Astrophysical Journal Letters

References in corpus (4)

• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• Massive Stars in the Quintuplet Cluster
• Stellar spectroscopy far beyond the Local Group
• A Catalog of OB Associations in the spiral galaxy NGC 300

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