Keywords
H I Regions:OB Associations
OB Associations:H I Regions
OB Associations:H I Regions
How to Cite
Kinematics and distribution of interstellar H I in the region 290° ≤ l ≤ 320°, +3° ≤ b ≤ +17°. (1985). Revista Mexicana De Astronomía Y Astrofísica, 10(1), 159-170. https://astronomia.unam.mx/journals/rmxaa/article/view/1985rmxaa..10..159o
Abstract
The analysis of the region 290° ≤ l ≤ 320°, +3° ≤ b ≤ +17° reveals the presence of some H I features with filamentary characteristics and, particularly, the existence of a supershell in the Sagittarius-Carina arm. The region encloses a group of young OB stars known as the Lower Centaurus-Crux association. It is proposed that an elongated shape cloud would be related genetically with such a star association. The close relation of radiocontinuum emission and H I gas at large height above the galactic plane is shown.Similar Articles
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