Abstract
We have observed the bipolar post-asymptotic giant branch candidate OH 231.8+4.2, using the mid-infrared interferometer MIDI and the infrared camera with the adaptive optics system NACO on the Very Large Telescope. An unresolved core (
Original language | English |
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Pages (from-to) | L123-L126 |
Journal | Astrophysical Journal |
Volume | 646 |
Issue number | 2 |
DOIs | |
Publication status | Published - 1 Aug 2006 |
Keywords
- Dust, extinction
- Infrared: stars
- ISM: jets and outflows
- Stars: AGB and post-AGB
- Stars: mass loss