Abstract
The interstellar medium is enriched primarily by matter ejected from evolved low and intermediate mass stars. The outflows from these stars create a circumstellar envelope in which a rich gas-phase and dust-nucleation chemistry takes place. We observed the nearest carbon-rich evolved star, IRCâ+10216, using the PACS (55?210â\ensuremath\mu
| Original language | English (Ireland) |
|---|---|
| Journal | Astronomy and Astrophysics |
| Volume | 518 |
| Publication status | Published - 1 Jan 2010 |
Authors (Note for portal: view the doc link for the full list of authors)
- Authors
- L. Decin and J. Cernicharo and M. J. Barlow and P. Royer and B. Vandenbussche and R. Wesson and E. T. Polehampton and E. De Beck and M. Ag\'undez and J. A. D. L. Blommaert and M. Cohen and F. Daniel and W. De Meester and K. Exter and H. Feuchtgruber and J. P. Fonfr\'ia and Walter Kieran Gear and J. R. Goicoechea and Haley Louise Gomez and M. A. T. Groenewegen and Peter Charles Hargrave and R. Huygen and P. Imhof and R. J. Ivison and C. Jean and F. Kerschbaum and S. J. Leeks and T. Lim and Mikako Matsuura and G. Olofsson and T. Posch and S. Regibo and G. Savini and B. Sibthorpe and B. M. Swinyard and B. Tercero and C. Waelkens and D. K. Witherick and J. A. Yates