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IRC +10 216 in 3-D: morphology of a TP-AGB star envelope
During their late pulsating phase, AGB stars expel most of their mass in the form of massive dusty envelopes, an event that largely controls the composition of interstellar matter. The envelopes, however, are distant and opaque to visible and NIR radiation: their structure remains poorly known and t...
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| Publicado no: | Astron Astrophys |
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| Main Authors: | , , , , , , , , , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
2018
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5815495/ https://ncbi.nlm.nih.gov/pubmed/29456257 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1051/0004-6361/201731619 |
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