L. M. Oskinova

TL;DR: In this article, a spectroscopic study of 320 massive stars of spectral types O (23 stars) and B (297 stars) in the Wing of the Small Magellanic Cloud (SMC) was performed using state-of-the-art stellar atmosphere models.

TL;DR: In this paper, the authors reported a clearly detected periodic X-ray flux variability with amplitude ~20% in the ASCA passband (0.5-10 keV).

TL;DR: In this paper, K-band integral-field spectroscopy was used to analyze four Wolf-Rayet stars of the nitrogen sequence (WN) found in the inner part of the Quintuplet cluster.

TL;DR: In this paper, the authors provide grids of model atmospheres for OB-type stars at metallicities corresponding to the Small and Large Magellanic Clouds, as well as to solar metallicity.

TL;DR: In this paper, a spectroscopic study of 320 OB stars in the Small Magellanic Cloud (SMC) was performed using state-of-the-art stellar atmosphere models, which revealed that in metal-poor environments the stellar feedback is dominated by corecollapse supernovae in combination with winds and ionizing radiation supplied by a few of the most massive stars.