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 |
|---|---|
| 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