A&A 625, A104 (2019) Astronomy https://doi.org/10.1051/0004-6361/201935365 & c ESO 2019 Astrophysics Testing massive star evolution, star formation history, and feedback at low metallicity Spectroscopic analysis of OB stars in the SMC Wing?,?? V. Ramachandran1, W.-R. Hamann1, L. M. Oskinova1,2, J. S. Gallagher3, R. Hainich1, T. Shenar4, A. A. C. Sander5, H. Todt1, and L. Fulmer6,7 1 Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Str. 24/25, 14476 Potsdam, Germany e-mail:
[email protected] 2 Kazan Federal University, Kremlevskaya Ul. 18, Kazan, Russia 3 Department of Astronomy, University of Wisconsin, Madison, WI, USA 4 Institute of Astrophysics, KU Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium 5 Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, UK 6 National Optical Astronomy Observatory, 950 North Cherry Ave., Tucson, AZ 85719, USA 7 University of Washington, Physics-Astronomy Bldg. 3910 15th Ave NE Rm. C319, Seattle, WA 98195, USA Received 20 February 2019 / Accepted 4 April 2019 ABSTRACT Stars that start their lives with spectral types O and early B are the progenitors of core-collapse supernovae, long gamma-ray bursts, neutron stars, and black holes. These massive stars are the primary sources of stellar feedback in star-forming galaxies. At low metallicities, the properties of massive stars and their evolution are not yet fully explored. Here we report 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). The spectra, which we obtained with the ESO Very Large Telescope, were analyzed using state-of-the-art stellar atmosphere models, and the stellar parameters were determined.