Centimetre-wave continuum radiation from the rho Ophiuchi molecular cloud

Centimetre-wave continuum radiation from the rho Ophiuchi molecular cloud

The ρ Oph molecular cloud is undergoing intermediate-mass star formation. Ultraviolet radiation from its hottest young stars heats and dissociates exposed layers, but does not ionize hydrogen. Only faint radiation from the Rayleigh-Jeans tail of ∼10-100 K dust is expected at wavelengths longwards of...

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Bibliographic Details
Main Authors:	Casassus, S, Dickinson, C, Cleary, K, Paladini, R, Etxaluze, M, Lim, T, White, G, Burton, M, Indermuehle, B, Stahl, O, Roche, P
Format:	Journal article
Language:	English
Published:	2008

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