Stellar Disk Evolution and Gaseous Disk Turbulence of Dwarf Irregular Galaxies

Name: Stellar Disk Evolution and Gaseous Disk Turbulence of Dwarf Irregular Galaxies
Brand: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG
SKU: 9783662570890
Price: 100.0 EUR
Availability: InStock

Autor: HONG-XIN ZHANG

Jazyk:

Väzba: Brožovaná

Vydavateľ: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG

Dostupnosť: Skladom u dodávateľa

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100.00 €

This book focuses on the stellar disk evolution and gas disk turbulence of the most numerous galaxie...

Informácie o knihe

Autor

HONG-XIN ZHANG

Jazyk

Angličtina

Väzba

Kniha - Brožovaná

Vydalo

2018

Stránok

165

EAN

9783662570890

ISBN

9783662570890

Enbook ID

19755982

Vydavateľ

Springer-Verlag Berlin and Heidelberg GmbH & Co. KG

Hmotnosť

454

Rozmery

155 x 235 x 11

Kompletný popis

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.

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