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A 2D view of Wolf-Rayet Galaxies

  • The main objective of this work is to investigate the evolution of massive stars, and the interplay between them and the ionized gas for a sample of local metal-poor Wolf-Rayet galaxies. Optical integral field spectrocopy was used in combination with multi-wavelength radio data. Combining optical and radio data, we locate Wolf-Rayet stars and supernova remnants across the Wolf-Rayet galaxies to study the spatial correlation between them. This study will shed light on the massive star formation and its feedback, and will help us to better understand distant star-forming galaxies.

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Author details:S. Srivastava, C. Kehrig, N. G. Kantharia, E. Pérez-Montero, J. M. Vílchez, J. Iglesias-Páramo, P. Janardhan
URN:urn:nbn:de:kobv:517-opus4-87650
Title of parent work (English):Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015
Publication type:Article
Language:English
Publication year:2015
Publishing institution:Universität Potsdam
Release date:2016/02/19
First page:59
Last Page:62
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
DDC classification:5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften
Publishing method:Universitätsverlag Potsdam
Collection(s):Universität Potsdam / Tagungsbände/Proceedings (nicht fortlaufend) / Wolf-Rayet Stars: Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 / Wolf-Rainer Hamann, Andreas Sander, Helge Todt (Eds.)
Universität Potsdam / Tagungsbände/Proceedings (nicht fortlaufend) / Wolf-Rayet Stars: Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 / Wolf-Rainer Hamann, Andreas Sander, Helge Todt (Eds.) / WR surveys
License (German):License LogoKeine öffentliche Lizenz: Unter Urheberrechtsschutz
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