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OverviewFull Product DetailsAuthor: Julia BodensteinerPublisher: Springer International Publishing AG Imprint: Springer International Publishing AG Edition: 1st ed. 2022 Weight: 0.237kg ISBN: 9783031194917ISBN 10: 3031194918 Pages: 128 Publication Date: 02 December 2023 Audience: Professional and scholarly , Professional & Vocational Format: Paperback Publisher's Status: Active Availability: Manufactured on demand  We will order this item for you from a manufactured on demand supplier. Table of ContentsIntroduction.- Spectroscopy of massive stars.- On the lack of main-sequence companions to massive Be stars.- Is HR 6819 a triple system containing a black hole? - An alternative explanation.- The young massive Small Magellanic Cloud Clusters NGC 330 seen by MUSE.- Summary and future work.- Appendices.ReviewsAuthor InformationJulia Bodensteiner is a postdoctoral researcher at the European Southern Observatory (ESO) in Garching by Munich, Germany. She began her academic career at the Technical University of Munich (TUM), Germany, and studied at the Universidad Complutense de Madrid, Spain, for one year during her bachelor’s degree. She then continued with a master degree at the TUM and successfully completed a collaborative Master’s thesis between the Max Planck Institute for Extraterrestrial Physics and the European Southern Observatory, focusing on observational astrophysics. For her Ph.D. thesis, Julia worked with Prof. Hugues Sana at the Institute of Astronomy at KU Leuven, Belgium. Her main research interests lie in the observational characterization of massive stars, with emphasize on the impact of stellar multiplicity on the evolution of stars and an observational approach to test and refine evolution theories of massive single and multiple stars. Tab Content 6Author Website:Countries AvailableAll regions |
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