Molecular cloud
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- Dark Supernova Remnants Revealed by CO-Line Bubbles in the W43 Molecular Complex Along the 4-Kpc Galactic Arm
- NL#150 January/February
- Star Formation
- Arxiv:2006.01326V1 [Astro-Ph.GA] 2 Jun 2020 58090 Morelia, Michoacan, Mexico
- A New Radio Molecular Line Survey of Planetary Nebulae HNC/HCN As a Diagnostic of Ultraviolet Irradiation J
- Interstellar Medium (ISM) Star Formation Formation of Planetary Systems 5.1 Interstellar Medium: General Properties
- Abundance of Iron-60 in Molecular Clouds N
- Relevance for Galactic Enrichment and Solar System Formation
- Star Formation and Molecular Clouds Towards the Galactic Anti-Center
- The Link Between Molecular Cloud Structure and Turbulence
- Dust-Temperature of an Isolated Star-Forming Cloud: Herschel
- Stellar Evolution – Cosmic Cycles of Formation and Destruction
- Stellar Evolution CESAR’S Booklet
- Planet Formation
- Presolar Cloud Collapse and the Formation and Early Evolution of the Solar Nebula
- Lecture 22 Physical Properties of Molecular Clouds
- A Compact Steep Spectrum Radio Source in NGC 1977 (Research Note)
- 10. the Lives of the Stars