2006/11/09 by Dimitris Stamatellos, D. Stamatellos, D. Ward–Thompson +4
Chemistry · Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Biology #Genetics #Molecular Spectroscopy and Structure #Nature versus nurture #Optics #Physics #Protostar #Star formation #Stars #Stellar, planetary, and galactic studies #Wavelength #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066387
Accepted by A&A
arxiv created 2006/11/09 · openalex publication_date 2006/11/13 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims.Four dense cores, L1582A, L1689A, B133 and B68, classified as prestellar in terms of the absence of detectable NIR emission, are observed at radio wavelengths to investigate whether they nurture very young protostars.