Abstract
Molecular outflows associated with GL 2591 and W28 A2 were observed in the 492 GHz [C I] line. Upper limits are set on the [C I] emission in the extremely high velocity line wings. These limits are discussed in terms of wind-driven and jet-driven models of molecular outflows.
Original language | English (US) |
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Pages (from-to) | 734-737 |
Number of pages | 4 |
Journal | Astrophysical Journal |
Volume | 435 |
Issue number | 2 |
DOIs | |
State | Published - Nov 10 1994 |
Keywords
- ISM : jets and outflows
- ISM: atoms
- ISM: individual (GL 2591, W28 A2)
- ISM: kinematics and dynamics
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science