A young double stellar cluster in an HII region, emerging from its parent molecular cloud

2008/03/04 by Joao L. Yun, J. L. Yun, Anlaug Amanda Djupvik +5
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20079090

15 pages, 16 figures

arxiv created 2008/03/04 · openalex publication_date 2008/03/19 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31

Abstract

Aims. We investigate the star formation occurring in the region towards IRAS 07141-0920 contained in the HII region Sh2-294 (S294). We report the discovery of a new young double stellar cluster, and we describe its properties.

Citations

• Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting Observed SEDs Using a Large Grid of Precomputed Models
• A multiwavelength study of Galactic HII region Sh2-294
• SpitzerObservations of the Orion OB1 Association: Second‐Generation Dust Disks at 5–10 Myr
• The Two Micron All Sky Survey (2MASS)
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• Formation scenarios for the young stellar associations between galactic longitudes l \mathsf= 280\degr-360\degr