Open AccessA Jet–driven, Extreme High‐Velocity Outflow Powered by a Cold, Low‐Luminosity Protostar near NGC 2023
Author(s) -
G. Sandell,
L. W. Avery,
F. Baas,
I. M. Coulson,
W. R. F. Dent,
Per Friberg,
W. P. K. Gear,
J. S. Greaves,
W. S. Holland,
T. Jenness,
P. R. Jewell,
J. F. Lightfoot,
H. E. Matthews,
G. H. MoriartySchieven,
Richard Prestage,
E. I. Robson,
J. A. Stevens,
R. P. J. Tilanus,
G. D. Watt
Publication year - 1999
Publication title -
the astrophysical journal
Language(s) - Uncategorized
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/307367
Subject(s) - outflow , physics , astrophysics , protostar , submillimeter array , bipolar outflow , astronomy , luminosity , serpens , millimeter , molecular cloud , star formation , stars , galaxy , meteorology
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