2014/05/22 by Marko M. Mäkelä, M. M. Mäkelä, L. K. Haikala +1 · 8 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Biology #Context (archaeology) #Galaxies: Formation, Evolution, Phenomena #Infrared #Paleontology #Physics #Rosette (schizont appearance) #Stars #Stellar, planetary, and galactic studies #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201423440
published in Astronomy and Astrophysics 567, A108 (EDP Sciences) · Accepted for publication in A&A. 24 pages, 27 figures. JHKs photometry will be available electronically
arxiv created 2014/05/22 · openalex publication_date 2014/06/11 · arxiv updated 2014/09/05 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Context. Giant galactic H ii regions surrounding central young clusters show compressed molecular shells, which have broken up into clumps, filaments, and elephant trunks interacting with UV light from central OB stars. Tiny, dense clumps of subsolar mass, called globulettes, form in this environment.