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Description du livre Hardcover. Etat : new. N° de réf. du vendeur 9783662528655
Description du livre Etat : New. N° de réf. du vendeur ABLIING23Mar3113020316928
Description du livre Etat : New. PRINT ON DEMAND Book; New; Fast Shipping from the UK. No. book. N° de réf. du vendeur ria9783662528655_lsuk
Description du livre Buch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This book focuses on the stellar disk evolution and gas disk turbulence of the most numerous galaxies in the local Universe - the dwarf galaxies. The 'outside-in' disk shrinking mode was established for a relatively large sample of dwarf galaxies for the first time, and this is in contrast to the 'inside-out' disk growth mode found for spiral galaxies. Double exponential brightness profiles also correspond to double exponential stellar mass profiles for dwarf galaxies, which is again different from most spiral galaxies. The cool gas distribution in dwarf galaxies was probed with the spatial power spectra of hydrogen iodide (HI) gas emission, and provided indirect evidence that inner disks of dwarf galaxies have proportionally more cool gas than outer disks. The finding that no correlation exists between gas power spectral indices and star formation gave important constraints on the relation between turbulence and star formation in dwarf galaxies. 188 pp. Englisch. N° de réf. du vendeur 9783662528655
Description du livre Gebunden. Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Nominated as an outstanding thesis by University of Chinese Academy of SciencesEstablishes the outside-in disk growth mode for most nearby dwarf irregular galaxiesDisproves the existence of a correlation between gas spatial power spectral. N° de réf. du vendeur 122021778
Description du livre Buch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - This book focuses on the stellar disk evolution and gas disk turbulence of the most numerous galaxies in the local Universe - the dwarf galaxies. The 'outside-in' disk shrinking mode was established for a relatively large sample of dwarf galaxies for the first time, and this is in contrast to the 'inside-out' disk growth mode found for spiral galaxies. Double exponential brightness profiles also correspond to double exponential stellar mass profiles for dwarf galaxies, which is again different from most spiral galaxies. The cool gas distribution in dwarf galaxies was probed with the spatial power spectra of hydrogen iodide (HI) gas emission, and provided indirect evidence that inner disks of dwarf galaxies have proportionally more cool gas than outer disks. The finding that no correlation exists between gas power spectral indices and star formation gave important constraints on the relation between turbulence and star formation in dwarf galaxies. N° de réf. du vendeur 9783662528655