2 papers
astro-ph.SR2026
Complex morphology and kinematics at the heart of the very low luminosity object IRAM 04191+1522
N. Otten, I. de Gregorio-Monsalvo, N. Huélamo +3
The formation of the majority of brown dwarfs (BDs) remains uncertain. They may form in molecular cloud cores in a process akin to low mass star formation, or via fragmentation in…
astro-ph.SR2026
IRAM 04191+1522: a compact proto-brown dwarf binary candidate
N. Huélamo, I. de Gregorio-Monsalvo, Aina Palau +12
Very low-luminosity objects in nearby star-forming regions have been identified as promising proto-brown dwarf candidates. The study of their multiplicity can shed light on the dom…