Detection of CH+ emission from the disc around HD 100546
Astronomy and Astrophysics 530 (2011): L2 Reproduced with permission from Astronomy & Astrophysics
| Autores: | , , , , , , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Fecha de publicación: | 2011 |
| País: | España |
| Institución: | Universidad Autónoma de Madrid |
| Repositorio: | Biblos-e Archivo. Repositorio Institucional de la UAM |
| Idioma: | inglés |
| OAI Identifier: | oai:repositorio.uam.es:10486/662190 |
| Acceso en línea: | http://hdl.handle.net/10486/662190 https://dx.doi.org/10.1051/0004-6361/201116678 |
| Access Level: | acceso abierto |
| Palabra clave: | Astrochemistry Protoplanetary disks Física |
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Detection of CH+ emission from the disc around HD 100546Thi, Wing FaiMénard, François C.Meeus, GwendolynMartin-Zaïdi, C.Woitke, PeterTatulli, EricBenisty, MyriamKamp, IngaPascucci, IlariaPinte, ChristopheGrady, Carol A.Brittain, Sean D.White, Glenn J.Howard, Christian D.Sandell, Göran H LEiroa, CarlosAstrochemistryProtoplanetary disksFísicaAstronomy and Astrophysics 530 (2011): L2 Reproduced with permission from Astronomy & AstrophysicsDespite its importance in the thermal balance of the gas and in the determination of primeval planetary atmospheres, the chemistry in protoplanetary discs remains poorly constrained with only a handful of detected species. We observed the emission from the disc around the Herbig Be star HD 100546 with the PACS instrument in the spectroscopic mode on board the Herschel Space Telescope as part of the GAS in Protoplanetary Systems (GASPS) programme and used archival data from the DIGIT programme to search for the rotational emission of CH+. We detected in both datasets an emission line centred at 72.16 μm that most likely corresponds to the J = 5−4 rotational emission of CH+. The J = 3−2 and 6−5 transitions are also detected albeit with lower confidence. Other CH+ rotational lines in the PACS observations are blended with water lines. A rotational diagram analysis shows that the CH+ gas is warm at 323+2320 −151 K with a mass of ∼3×10−14−5×10−12 M_.We modelled the CH+ chemistry with the chemo-physical code ProDiMo using a disc density structure and grain parameters that match continuum observations and near- and mid-infrared interferometric data. The model suggests that CH+ is most abundant at the location of the disc rim at 10−13 AU from the star where the gas is warm, which is consistent with previous observations of hot CO gas emissionThis work is partly supported by the Spanish grant AYA 2008-01727. Also is funding from the EC 7th Framework Programme (PIEF-GA-2008-220891, PERG06- GA-2009-256513)ESODepartamento de Física TeóricaFacultad de Ciencias20112011-05-04research articlehttp://purl.org/coar/resource_type/c_2df8fbb1VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10486/662190https://dx.doi.org/10.1051/0004-6361/201116678reponame:Biblos-e Archivo. Repositorio Institucional de la UAMinstname:Universidad Autónoma de MadridInglésengEuropean Commission http://dx.doi.org/10.13039/501100000780 Framework Programme Seven 220891open accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:repositorio.uam.es:10486/6621902026-06-23T12:46:27Z |
| dc.title.none.fl_str_mv |
Detection of CH+ emission from the disc around HD 100546 |
| title |
Detection of CH+ emission from the disc around HD 100546 |
| spellingShingle |
Detection of CH+ emission from the disc around HD 100546 Thi, Wing Fai Astrochemistry Protoplanetary disks Física |
| title_short |
Detection of CH+ emission from the disc around HD 100546 |
| title_full |
Detection of CH+ emission from the disc around HD 100546 |
| title_fullStr |
Detection of CH+ emission from the disc around HD 100546 |
| title_full_unstemmed |
Detection of CH+ emission from the disc around HD 100546 |
| title_sort |
Detection of CH+ emission from the disc around HD 100546 |
| dc.creator.none.fl_str_mv |
Thi, Wing Fai Ménard, François C. Meeus, Gwendolyn Martin-Zaïdi, C. Woitke, Peter Tatulli, Eric Benisty, Myriam Kamp, Inga Pascucci, Ilaria Pinte, Christophe Grady, Carol A. Brittain, Sean D. White, Glenn J. Howard, Christian D. Sandell, Göran H L Eiroa, Carlos |
| author |
Thi, Wing Fai |
| author_facet |
Thi, Wing Fai Ménard, François C. Meeus, Gwendolyn Martin-Zaïdi, C. Woitke, Peter Tatulli, Eric Benisty, Myriam Kamp, Inga Pascucci, Ilaria Pinte, Christophe Grady, Carol A. Brittain, Sean D. White, Glenn J. Howard, Christian D. Sandell, Göran H L Eiroa, Carlos |
| author_role |
author |
| author2 |
Ménard, François C. Meeus, Gwendolyn Martin-Zaïdi, C. Woitke, Peter Tatulli, Eric Benisty, Myriam Kamp, Inga Pascucci, Ilaria Pinte, Christophe Grady, Carol A. Brittain, Sean D. White, Glenn J. Howard, Christian D. Sandell, Göran H L Eiroa, Carlos |
| author2_role |
author author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
Departamento de Física Teórica Facultad de Ciencias |
| dc.subject.none.fl_str_mv |
Astrochemistry Protoplanetary disks Física |
| topic |
Astrochemistry Protoplanetary disks Física |
| description |
Astronomy and Astrophysics 530 (2011): L2 Reproduced with permission from Astronomy & Astrophysics |
| publishDate |
2011 |
| dc.date.none.fl_str_mv |
2011 2011-05-04 |
| dc.type.none.fl_str_mv |
research article http://purl.org/coar/resource_type/c_2df8fbb1 VoR http://purl.org/coar/version/c_970fb48d4fbd8a85 |
| dc.type.openaire.fl_str_mv |
info:eu-repo/semantics/article |
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article |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10486/662190 https://dx.doi.org/10.1051/0004-6361/201116678 |
| url |
http://hdl.handle.net/10486/662190 https://dx.doi.org/10.1051/0004-6361/201116678 |
| dc.language.none.fl_str_mv |
Inglés eng |
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Inglés |
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eng |
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European Commission http://dx.doi.org/10.13039/501100000780 Framework Programme Seven 220891 |
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open access http://purl.org/coar/access_right/c_abf2 |
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info:eu-repo/semantics/openAccess |
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open access http://purl.org/coar/access_right/c_abf2 |
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openAccess |
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