Structure and stability in TMC-1: Analysis of NH3molecular line andHerschelcontinuum data

2016/03/18 by O. Fehér, L. V. Tóth, D. Ward-Thompson +6
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Balmer series #Computational astrophysics #Emission spectrum #Line (geometry) #Molecular cloud #Morphology (biology) #Stability (learning theory) #Star (game theory) #Stellar, planetary, and galactic studies #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201424385

published as A&A 590, A75 (2016) · 17 pages, 9 figures; accepted for publication in A&A

arxiv created 2016/03/18 · openalex publication_date 2016/03/28 · arxiv updated 2016/05/18 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We examined the velocity, density, and temperature structure of Taurus molecular cloud-1 (TMC-1), a filamentary cloud in a nearby quiescent star forming area, to understand its morphology and evolution.

Citations

• Silhouettes: A graphical aid to the interpretation and validation of cluster analysis
• Structure Function Scaling of a 2MASS Extinction Map of Taurus
• The Five College Radio Astronomy Observatory CO Mapping Survey of the Taurus Molecular Cloud
• HST/NICMOS observations of a proto-brown dwarf candidate
• Chains of dense cores in the Taurus L1495/B213 complex
• Similarity Analysis by Reciprocal Pairs for Discrete and Continuous Data
• Structural Analysis of Molecular Clouds: Dendrograms
• Interstellar Ammonia