Abstract
Gradients in molecular abundances along the TMC-1 ridge have been observed by several authors, most recently in a comprehensive study by Pratap et al. These can be explained by there being a difference in density, C/O ratio, or chemical evolutionary state along the ridge. The presence at the carbon-rich
Original language | English |
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Pages (from-to) | 256-265 |
Number of pages | 10 |
Journal | Astrophysical Journal |
Volume | 535 |
Issue number | 1 PART 1 |
Publication status | Published - 20 May 2000 |
ASJC Scopus subject areas
- Space and Planetary Science