The mode of gas accretion onto star-forming galaxies
It is argued that galaxies like ours sustain their star formation by transferring gas from an extensive corona to the star-forming disc. The transfer is effected by the galactic fountain -- cool clouds that are shot up from the plane to kiloparsec heights above the plane. The Kelvin-Helmholtz instab...
| Asıl Yazarlar: | , , , , , |
|---|---|
| Materyal Türü: | Journal article |
| Baskı/Yayın Bilgisi: |
2010
|
Search Result 1
