| Issue |
EPJ Web of Conferences
Volume 265, 2022
Multi-line Diagnostics of the Interstellar Medium
|
|
|---|---|---|
| Article Number | 00029 | |
| Number of page(s) | 6 | |
| DOI | https://doi.org/10.1051/epjconf/202226500029 | |
| Published online | 07 September 2022 | |
https://doi.org/10.1051/epjconf/202226500029
Molecules from evolved stars and their role in the cycle of the ISM
Instituto de Física Fundamental, CSIC, Calle Serrano 123, 28006 Madrid, Spain
* e-mail: marcelino.agundez@csic.es
Published online: 7 September 2022
The ejecta of evolved stars are among the most efficient chemical laboratories in the Universe. Many of the chemical compounds synthesized in these environments probably travel along the interstellar medium and may be ultimately delivered to planets. However, we still do not understand many of the chemical processes at work during the evolution from the AGB phase to the PN. Here we review key aspects of our current understanding of the chemistry of AGB and post-AGB envelopes, highlighting the issues that are yet to be understood.
© The Authors, Published by EDP Sciences, 2022
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
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