Authors:
- Nominated as an outstanding thesis by University of Chinese Academy of Sciences
- Establishes the "outside-in" disk growth mode for most nearby dwarf irregular galaxies
- Disproves the existence of a correlation between gas spatial power spectral indices and star formation in galaxies
- Provides indirect evidence that inner disks of dwarf galaxies have proportionally more cool gas
- Includes supplementary material: sn.pub/extras
Part of the book series: Springer Theses (Springer Theses)
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Table of contents (5 chapters)
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Front Matter
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Back Matter
About this book
Authors and Affiliations
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Pontificia Universidad Catolica de Chile, Instituto de Astrofísica, Facultad de Física, Santiago, Chile
Hong-Xin Zhang
About the author
Bibliographic Information
Book Title: Stellar Disk Evolution and Gaseous Disk Turbulence of Dwarf Irregular Galaxies
Authors: Hong-Xin Zhang
Series Title: Springer Theses
DOI: https://doi.org/10.1007/978-3-662-52867-9
Publisher: Springer Berlin, Heidelberg
eBook Packages: Physics and Astronomy, Physics and Astronomy (R0)
Copyright Information: Springer-Verlag Berlin Heidelberg 2016
Hardcover ISBN: 978-3-662-52865-5Published: 02 September 2016
Softcover ISBN: 978-3-662-57089-0Published: 15 June 2018
eBook ISBN: 978-3-662-52867-9Published: 27 August 2016
Series ISSN: 2190-5053
Series E-ISSN: 2190-5061
Edition Number: 1
Number of Pages: XIX, 165
Number of Illustrations: 15 b/w illustrations, 35 illustrations in colour