Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discs

Astronomy and Astrophysics 544 (2012): A78 Reproduced with permission from Astronomy & Astrophysics

Detalles Bibliográficos
Autores: Meeus, Gwendolyn, Montesinos, Benjamín, Mendigutía, I., Kamp, Inga, Thi, Wing Fai, Eiroa, Carlos, Grady, Carol A., Mathews, Geoffrey, Sandell, Göran, Martin-Zaïdi, C., Brittain, Sean, Dent, William R F, Howard, Christian, Ménard, François C., Pinte, Christophe, Roberge, Aki, Vandenbussche, Bart, Williams, Jonathan P.
Tipo de recurso: artículo
Fecha de publicación:2012
País:España
Institución:Universidad Autónoma de Madrid
Repositorio:Biblos-e Archivo. Repositorio Institucional de la UAM
Idioma:inglés
OAI Identifier:oai:repositorio.uam.es:10486/662206
Acceso en línea:http://hdl.handle.net/10486/662206
https://dx.doi.org/10.1051/0004-6361/201219225
Access Level:acceso abierto
Palabra clave:Astrochemistry
Circumstellar matter
Line: identification
Planetary systems
Protoplanetary disks
Física
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oai_identifier_str oai:repositorio.uam.es:10486/662206
network_acronym_str ES
network_name_str España
repository_id_str
dc.title.none.fl_str_mv Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discs
title Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discs
spellingShingle Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discs
Meeus, Gwendolyn
Astrochemistry
Circumstellar matter
Line: identification
Planetary systems
Protoplanetary disks
Física
title_short Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discs
title_full Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discs
title_fullStr Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discs
title_full_unstemmed Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discs
title_sort Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discs
dc.creator.none.fl_str_mv Meeus, Gwendolyn
Montesinos, Benjamín
Mendigutía, I.
Kamp, Inga
Thi, Wing Fai
Eiroa, Carlos
Grady, Carol A.
Mathews, Geoffrey
Sandell, Göran
Martin-Zaïdi, C.
Brittain, Sean
Dent, William R F
Howard, Christian
Ménard, François C.
Pinte, Christophe
Roberge, Aki
Vandenbussche, Bart
Williams, Jonathan P.
author Meeus, Gwendolyn
author_facet Meeus, Gwendolyn
Montesinos, Benjamín
Mendigutía, I.
Kamp, Inga
Thi, Wing Fai
Eiroa, Carlos
Grady, Carol A.
Mathews, Geoffrey
Sandell, Göran
Martin-Zaïdi, C.
Brittain, Sean
Dent, William R F
Howard, Christian
Ménard, François C.
Pinte, Christophe
Roberge, Aki
Vandenbussche, Bart
Williams, Jonathan P.
author_role author
author2 Montesinos, Benjamín
Mendigutía, I.
Kamp, Inga
Thi, Wing Fai
Eiroa, Carlos
Grady, Carol A.
Mathews, Geoffrey
Sandell, Göran
Martin-Zaïdi, C.
Brittain, Sean
Dent, William R F
Howard, Christian
Ménard, François C.
Pinte, Christophe
Roberge, Aki
Vandenbussche, Bart
Williams, Jonathan P.
author2_role author
author
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
Circumstellar matter
Line: identification
Planetary systems
Protoplanetary disks
Física
topic Astrochemistry
Circumstellar matter
Line: identification
Planetary systems
Protoplanetary disks
Física
description Astronomy and Astrophysics 544 (2012): A78 Reproduced with permission from Astronomy & Astrophysics
publishDate 2012
dc.date.none.fl_str_mv 2012
2012-08-08
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
format article
dc.identifier.none.fl_str_mv http://hdl.handle.net/10486/662206
https://dx.doi.org/10.1051/0004-6361/201219225
url http://hdl.handle.net/10486/662206
https://dx.doi.org/10.1051/0004-6361/201219225
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.relation.none.fl_str_mv European Commission http://dx.doi.org/10.13039/501100000780 Framework Programme Seven 284405
European Commission http://dx.doi.org/10.13039/501100000780 Framework Programme Seven 256513
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv ESO
publisher.none.fl_str_mv ESO
dc.source.none.fl_str_mv reponame:Biblos-e Archivo. Repositorio Institucional de la UAM
instname:Universidad Autónoma de Madrid
instname_str Universidad Autónoma de Madrid
reponame_str Biblos-e Archivo. Repositorio Institucional de la UAM
collection Biblos-e Archivo. Repositorio Institucional de la UAM
repository.name.fl_str_mv
repository.mail.fl_str_mv
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spelling Observations of Herbig Ae/Be stars with Herschel/PACS: The atomic and molecular contents of their protoplanetary discsMeeus, GwendolynMontesinos, BenjamínMendigutía, I.Kamp, IngaThi, Wing FaiEiroa, CarlosGrady, Carol A.Mathews, GeoffreySandell, GöranMartin-Zaïdi, C.Brittain, SeanDent, William R FHoward, ChristianMénard, François C.Pinte, ChristopheRoberge, AkiVandenbussche, BartWilliams, Jonathan P.AstrochemistryCircumstellar matterLine: identificationPlanetary systemsProtoplanetary disksFísicaAstronomy and Astrophysics 544 (2012): A78 Reproduced with permission from Astronomy & AstrophysicsWe observed a sample of 20 representative Herbig Ae/Be stars and 5 A-type debris discs with PACS onboard Herschel, as part of the GAS in Protoplanetary Systems (GASPS) project. The observations were done in spectroscopic mode, and cover the far-infrared lines of [O i], [C ii], CO, CH+, H2O, and OH. We have a [Oi] 63 μm detection rate of 100% for the Herbig Ae/Be and 0% for the debris discs. The [Oi] 145 μm line is only detected in 25% and CO J = 18–17 in 45% (and fewer cases for higher J transitions) of the Herbig Ae/Be stars, while for [Cii] 157 μm, we often find spatially variable background contamination. We show the first detection of water in a Herbig Ae disc, HD 163296, which has a settled disc. Hydroxyl is detected as well in this disc. First seen in HD 100546, CH+ emission is now detected for the second time in a Herbig Ae star, HD 97048. We report fluxes for each line and use the observations as line diagnostics of the gas properties. Furthermore, we look for correlations between the strength of the emission lines and either the stellar or disc parameters, such as stellar luminosity, ultraviolet and X-ray flux, accretion rate, polycyclic aromatic hydrocarbon (PAH) band strength, and flaring. We find that the stellar ultraviolet flux is the dominant excitation mechanism of [Oi] 63 μm, with the highest line fluxes being found in objects with a large amount of flaring and among the largest PAH strengths. Neither the amount of accretion nor the X-ray luminosity has an influence on the line strength. We find correlations between the line flux of [Oi] 63 μm and [Oi] 145 μm, CO J = 18–17 and [Oi] 6300 Å, and between the continuum flux at 63 μm and at 1.3 mm, while we find weak correlations between the line flux of [O i] 63 μm and the PAH luminosity, the line flux of CO J = 3–2, the continuum flux at 63 μm, the stellar effective temperature, and the Brγ luminosity. Finally, we use a combination of the [O i] 63 μm and 12CO J = 2–1 line fluxes to obtain order of magnitude estimates of the disc gas masses, in agreement with the values that we find from detailed modelling of two Herbig Ae/Be stars, HD 163296 and HD 169142G. Meeus, C. Eiroa, I. Mendigutía, and B. Montesinos are partly supported by AYA-2008- 1727 and AYA-2011-26202. G. Meeus is supported by RYC-2011-07920. C.A.G. and S.D.B. acknowledge NASA/JPL for funding support. W.F.T. thanks CNES for financial support. F.M. thanks the Millennium Science Initiative (ICM) of the Chilean ministry of Economy (Nucleus P10-022-F). F.M., I.K., and W.F.T. acknowledge support from the EU FP7-2011 under Grant Agreement No. 284405. C.P. acknowledges funding from the EU FP7 under contract PERG06-GA-2009-256513 and from ANR of France under ontract ANR-2010-JCJC-0504-01. PACS has been developed by a consortium of institutes led by MPE (Germany) and including UVIE (Austria); KUL, CSL, IMEC (Belgium); CEA, OAMP (France); MPIA (Germany); IFSI, OAP/AOT, OAA/CAISMI, LENS, SISSA (Italy); IAC (Spain). This development has been supported by the funding agencies BMVIT (Austria), ESA-PRODEX (Belgium), CEA/CNES (France), DLR (Germany), ASI (Italy), and CICT/MCT (Spain). This research has made use of the SIMBAD database, operated at CDS, Strasbourg, FranceESODepartamento de Física TeóricaFacultad de Ciencias20122012-08-08research articlehttp://purl.org/coar/resource_type/c_2df8fbb1VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10486/662206https://dx.doi.org/10.1051/0004-6361/201219225reponame:Biblos-e Archivo. Repositorio Institucional de la UAMinstname:Universidad Autónoma de MadridInglésengEuropean Commission http://dx.doi.org/10.13039/501100000780 Framework Programme Seven 284405European Commission http://dx.doi.org/10.13039/501100000780 Framework Programme Seven 256513open accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:repositorio.uam.es:10486/6622062026-06-23T12:46:27Z
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