Probing the initial conditions of high-mass star formation II : Fragmentation, stability, and chemistry towards high-mass star-forming regions G29.96-0.02 and G35.20-1.74

2011/04/11 by T. Pillai, J. Kauffmann, Jens Kauffmann +4 · 2 citations
Chemistry · Physics and Astronomy · #Accretion (finance) #Astrochemistry #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Fragmentation (computing) #Galaxy #Geology #High resolution #Infrared #Interstellar medium #Maser #Molecular Spectroscopy and Structure #Physics #Star formation #Stars #Stellar, planetary, and galactic studies #Turbulence #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201015899

accepted to A&A; Table 5 is affected by non-trivial arXiv typesetting problems

arxiv created 2011/04/29 · openalex publication_date 2011/06/01 · arxiv updated 2015/05/28 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/15

Abstract

Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory

Citations

• Identifying the Low‐Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores
• GLIMPSE. I. AnSIRTFLegacy Project to Map the Inner Galaxy
• Infall Collapse Solutions in the Inner Limit: Radiation Pressure and Its Effects on Star Formation
• Molecular Ions in L1544. II. The Ionization Degree
• Massive star formation in 100,000 years from turbulent and pressurized molecular clouds
• Conditions for the formation of massive stars
• The Formation of Massive Stars from Turbulent Cores
• First polarimetry results of two candidate high-mass protostellar objects
• Probing the formation of intermediate- to high-mass stars in protoclusters
• Probing the initial conditions of high mass star formation

Cited by

• Investigating the structure and fragmentation of a highly filamentary IRDC
• Deuterium fractionation and the degree of ionisation in massive clumps within infrared dark clouds