A Metal‐poor Compact HiiRegion with a Small, Isolated, and Dense Young Stellar Cluster
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/573/i=1/a=238/pdf
Reference31 articles.
1. Blitz, L. 1987, Physical Processes in Interstellar Clouds, ed. G. E. Morfill & M. Scholer (Dordrecht: Reidel), 35
2. High density molecular clumps around protostellar candidates
3. The NRAO VLA Sky Survey
4. Abundance analysis of giant H II regions in M51
5. M83 II: Spectral characteristics and chemical abundances of H II regions
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1. Molecular Cores and Young Clusters of Star Forming Regions;Chinese Astronomy and Astrophysics;2011-04
2. Massive Star Formation Triggered by Collision between Galactic and Accreted Intergalactic Clouds;The Astrophysical Journal;2004-09-17
3. IRAS 04000+5052: A Not So Compact, Not So Metal‐poor HiiRegion;Publications of the Astronomical Society of the Pacific;2004-08
4. Star Formation in Molecular Cloud Associated with IRAS 07028-1100;Chinese Physics Letters;2004-07-30
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