The high-mass star-forming region IRAS 18182-1433

2006/03/30 by H. Beuther, Q. Zhang, Qizhou Zhang +5 · 55 citations
Chemistry · Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Geology #High mass #High resolution #Molecular Spectroscopy and Structure #Physics #Remote sensing #Star (game theory) #Star formation #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20064887

published in Astronomy and Astrophysics 454(1), 221-231 (EDP Sciences) · Accepted for Astronomy and Astrophysics, 13 pages 13 figures. A version with high-resolution images can be found at http://www.mpia.de/homes/beuther/papers.html

arxiv created 2006/03/30 · openalex publication_date 2006/07/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.We present mm line and continuum observations at high spatial resolution characterizing the physical and chemical properties of the young massive star-forming region IRAS 18182-1433.

Citations

• High Spatial Resolution CN and CS Observation of Two Regions of Massive Star Formation

Cited by

• Unveiling the nature and interaction of the intermediate/high-mass YSOs in IRAS 20343+4129