Resolved 24.5 micron emission from massive young stellar objects

2008/11/25 by W. J. de Wit, M. G. Hoare, T. Fujiyoshi +15 · 69 citations
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Context (archaeology) #Geology #Physics #Star (game theory) #Star formation #Stars #Stellar, planetary, and galactic studies #Young stellar object #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810771

published in Astronomy and Astrophysics 494(1), 157-178 (EDP Sciences) · 21 pages, accepted for A&A

arxiv created 2008/11/25 · openalex publication_date 2008/12/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context. Massive young stellar objects (MYSO) are surrounded by massive dusty envelopes, whose physical structure and geometry are determined by the star formation process.

Citations

• A high-frequency radio continuum study of massive young stellar objects
• The size distribution of interstellar grains
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• NGC 2264 IRS 1: The Central Engine and Its Cavity
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Cited by

• SUBMILLIMETER ARRAY HIGH-ANGULAR RESOLUTION OBSERVATIONS OF THE MONOCEROS R2 STAR-FORMING CLUSTER
• The JCMT Spectral Legacy Survey: physical structure of the molecular envelope of the high-mass protostar AFGL2591