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PopIII-star siblings in IZw18 and metal-poor WR galaxies unveiled from integral field spectroscopy

  • Here, we highlight our recent results from the IFS study of Mrk178, the closest metal-poor WR galaxy, and of IZw18, the most metal-poor star-forming galaxy known in the local Universe. The IFS data of Mrk178 show the importance of aperture effects on the search for WR features, and the extent to which physical variations in the ISM properties can be detected. Our IFS data of IZw18 reveal its entire nebular HeIIλ4686-emitting region, and indicate for the very first time that peculiar, hot (nearly) metal-free ionizing stars (called here PopIII-star siblings) might hold the key to the HeII-ionization in IZw18.

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Author details:C. Kehrig, J. M. Vílchez, E. Pérez-Montero, J. Iglesias-Páramo, Jarle BrinchmannORCiD, P. A. Crowther, F. Durret, D. Kunth
URN:urn:nbn:de:kobv:517-opus4-87648
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:55
Last Page:58
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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