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(1 - 7 of 7)
How massive star FEEDBACK carves pillars out of dense gas
The impact of shocks on the chemistry of molecular clouds: high resolution images of chemical di_erentiation along the NGC 1333-IRAS 2A outow
Sub - arcsec imaging at 267 GHz of a young binary system: detection of a dust disk of radius less than 70 AU around T Tauri N
A molecular line study of NGC 1333 IRAS 4
Photon heating of envelopes around young stellar objects: an explanation for CO J=6-5 emission
Molecular abundances and low mass star formation I. Si-  and S- bearing species towards IRAS 16293-2422
Molecular abundances and low-mass star formation. 1: Si- and S-bearing species toward IRAS 16293-2422