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Probing chemical processes in AGB stars
| Content Provider | Scilit |
|---|---|
| Author | Schöier, Fredrik L. Olofsson, Hans |
| Copyright Year | 2008 |
| Description | We are conducting multi-transition observations of circumstellar line emission from common molecules such as HCN, SiO, CS, SiS and CN for a large sample of AGB stars with varying photospheric C/O-ratios and mass-loss charachteristics. Our recently published results for SiO and SiS clearly show that major constraints on the relative roles of non-equilibrium chemistry, dust condensation, and photodissociation can be obtained from the study of circumstellar molecular line emission. Presented here are also preliminary results based on detailed radiative transfer modelling of HCN line emission. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/4F741476D273E98C5374EEBA8A685A4C/S174392130802156Xa.pdf/div-class-title-probing-chemical-processes-in-agb-stars-div.pdf |
| Ending Page | 206 |
| Page Count | 6 |
| Starting Page | 201 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s174392130802156x |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | S251 |
| Volume Number | 4 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2008-02-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union Astronomy and Astrophysics agb Circumstellar Matter Mass Loss |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |