The Study of a System of H ii Regions toward L = 24.°8, B = 0.°1 at the Galactic Bar: Norma Arm Interface
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/866/i=1/a=20/pdf
Reference88 articles.
1. Collision between dissimilar clouds: stability of the bow-shock, and the formation of pre-stellar cores
2. RESOLUTION OF THE DISTANCE AMBIGUITY FOR GALACTIC H II REGIONS
3. THE MOLECULAR PROPERTIES OF GALACTIC H II REGIONS
4. Star formation triggered by non-head-on cloud–cloud collisions, and clouds with pre-collision sub-structure
5. STAR FORMATION AROUND MID-INFRARED BUBBLE N37: EVIDENCE OF CLOUD–CLOUD COLLISION
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