AB Aur: A Rosetta stone for planet formation theories
AB Aur is a Herbig Ae star that hosts a well-known protoplanetary disk that depicts a plethora of features that can be attributed to the presence of a forming planet, such as a large inner cavity, a dust trap, and spiral arms. We present NOEMA observations of molecular species towards this transitio...
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Format: | Article |
Language: | English |
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EDP Sciences
2022-01-01
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Series: | EPJ Web of Conferences |
Online Access: | https://www.epj-conferences.org/articles/epjconf/pdf/2022/09/epjconf_ism2022_00040.pdf |
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author | Rivière-Marichalar Pablo |
author_facet | Rivière-Marichalar Pablo |
author_sort | Rivière-Marichalar Pablo |
collection | DOAJ |
description | AB Aur is a Herbig Ae star that hosts a well-known protoplanetary disk that depicts a plethora of features that can be attributed to the presence of a forming planet, such as a large inner cavity, a dust trap, and spiral arms. We present NOEMA observations of molecular species towards this transition disk around AB Aur, including CO, 13CO, C18O, HCN, HCO+, SO, H2CO, and H2S. These observations reveal complex chemistry with strong chemical differentiation and the presence of a cavity-crossing filament. |
first_indexed | 2024-04-12T10:00:48Z |
format | Article |
id | doaj.art-62fc734feda34c60b181e6771a535d5b |
institution | Directory Open Access Journal |
issn | 2100-014X |
language | English |
last_indexed | 2024-04-12T10:00:48Z |
publishDate | 2022-01-01 |
publisher | EDP Sciences |
record_format | Article |
series | EPJ Web of Conferences |
spelling | doaj.art-62fc734feda34c60b181e6771a535d5b2022-12-22T03:37:34ZengEDP SciencesEPJ Web of Conferences2100-014X2022-01-012650004010.1051/epjconf/202226500040epjconf_ism2022_00040AB Aur: A Rosetta stone for planet formation theoriesRivière-Marichalar Pablo0Observatorio Astronómico Nacional (OAN,IGN)AB Aur is a Herbig Ae star that hosts a well-known protoplanetary disk that depicts a plethora of features that can be attributed to the presence of a forming planet, such as a large inner cavity, a dust trap, and spiral arms. We present NOEMA observations of molecular species towards this transition disk around AB Aur, including CO, 13CO, C18O, HCN, HCO+, SO, H2CO, and H2S. These observations reveal complex chemistry with strong chemical differentiation and the presence of a cavity-crossing filament.https://www.epj-conferences.org/articles/epjconf/pdf/2022/09/epjconf_ism2022_00040.pdf |
spellingShingle | Rivière-Marichalar Pablo AB Aur: A Rosetta stone for planet formation theories EPJ Web of Conferences |
title | AB Aur: A Rosetta stone for planet formation theories |
title_full | AB Aur: A Rosetta stone for planet formation theories |
title_fullStr | AB Aur: A Rosetta stone for planet formation theories |
title_full_unstemmed | AB Aur: A Rosetta stone for planet formation theories |
title_short | AB Aur: A Rosetta stone for planet formation theories |
title_sort | ab aur a rosetta stone for planet formation theories |
url | https://www.epj-conferences.org/articles/epjconf/pdf/2022/09/epjconf_ism2022_00040.pdf |
work_keys_str_mv | AT rivieremarichalarpablo abaurarosettastoneforplanetformationtheories |