New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)

[Aims]: We present the novel InterStellar Astrochemistry Chamber (ISAC), designed for studying solids (ice mantles, organics, and silicates) in interstellar and circumstellar environments: characterizing their physico-chemical properties and monitoring their evolution as caused by (i) vacuum-UV irra...

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Autores: Muñoz Caro, G.M., Jiménez-Escobar, A., Martín-Gago, José A., Rogero, Celia, Atienza, C., Puertas, S., Sobrado, Jesús Manuel, Torres-Redondo, Josefina
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2010
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/344271
Acceso en línea:http://hdl.handle.net/10261/344271
Access Level:acceso abierto
Palabra clave:ISM: clouds
ISM: molecules
Molecular processes
Methods: laboratory
Infrared: ISM
Techniques: spectroscopic
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spelling New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)Muñoz Caro, G.M.Jiménez-Escobar, A.Martín-Gago, José A.Rogero, CeliaAtienza, C.Puertas, S.Sobrado, Jesús ManuelTorres-Redondo, JosefinaISM: cloudsISM: moleculesMolecular processesMethods: laboratoryInfrared: ISMTechniques: spectroscopic[Aims]: We present the novel InterStellar Astrochemistry Chamber (ISAC), designed for studying solids (ice mantles, organics, and silicates) in interstellar and circumstellar environments: characterizing their physico-chemical properties and monitoring their evolution as caused by (i) vacuum-UV irradiation; (ii) cosmic ray irradiation; and (iii) thermal processing. Experimental study of thermal and photodesorption of the CO ice reported here simulates the freeze-out and desorption of CO on grains, providing new information on these processes. [Methods]: ISAC is an UHV set-up, with base pressure down to P = 2.5 × 10-11 mbar, where an ice layer is deposited at 7 K and can be UV-irradiated. The evolution of the solid sample was monitored by in situ transmittance FTIR spectroscopy, while the volatile species were monitored by QMS. [Results]: The UHV conditions of ISAC allow experiments under extremely clean conditions. Transmittance FTIR spectroscopy coupled to QMS proved to be ideal for in situ monitoring of ice processes that include radiation and thermal annealing. Thermal desorption of CO starting at 15 K, induced by the release of H2 from the CO ice, was observed. We measured the photodesorption yield of CO ice per incident photon at 7, 8, and 15 K, respectively yielding 6.4 ± 0.5 × 10-2, 5.4 ± 0.5 × 10-2, and 3.5 ± 0.5 × 10-2 CO molecules photon (7.3–10.5 eV)-1. Our value of the photodesorption yield of CO ice at 15 K is about one order of magnitude higher than the previous estimate. We confirmed that the photodesorption yield is constant during irradiation and independent of the ice thickness. Only below ~ 5 monolayers ice thickness the photodesorption rate decreases, which suggests that only the UV photons absorbed in the top 5 monolayers led to photodesorption. The measured CO photodesorption quantum yield at 7 K per absorbed photon in the top 5 monolayers is 3.4 molecules photon-1. [Conclusions]: Experimental values were used as input for a simple model of a quiescent cloud interior. Photodesorption seems to explain the observations of CO in the gas phase for densities below 3–7  × 104 cm-3. For the same density of a cloud, 3 × 104 cm-3, thermal desorption of CO is not triggered until T = 14.5 K. This has important implications for CO ice mantle build up in dark clouds.A.J.E. is supported by a research training grant from INTA. G.M.M.C. was financed by a Ramón y Cajal research contract from the MCYT in Spain. This work was supported by project AYA2008-06374 funded by Spanish MICINN.Peer reviewedEDP SciencesMinisterio de Ciencia y Tecnología (España)Ministerio de Ciencia e Innovación (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2024202420102024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/344271reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/MICINN//AYA2008-06374https://doi.org/10.1051/0004-6361/200912462Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3442712026-05-22T06:33:51Z
dc.title.none.fl_str_mv New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)
title New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)
spellingShingle New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)
Muñoz Caro, G.M.
ISM: clouds
ISM: molecules
Molecular processes
Methods: laboratory
Infrared: ISM
Techniques: spectroscopic
title_short New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)
title_full New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)
title_fullStr New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)
title_full_unstemmed New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)
title_sort New results on thermal and photodesorption of CO ice using the novel InterStellar Astrochemistry Chamber (ISAC)
dc.creator.none.fl_str_mv Muñoz Caro, G.M.
Jiménez-Escobar, A.
Martín-Gago, José A.
Rogero, Celia
Atienza, C.
Puertas, S.
Sobrado, Jesús Manuel
Torres-Redondo, Josefina
author Muñoz Caro, G.M.
author_facet Muñoz Caro, G.M.
Jiménez-Escobar, A.
Martín-Gago, José A.
Rogero, Celia
Atienza, C.
Puertas, S.
Sobrado, Jesús Manuel
Torres-Redondo, Josefina
author_role author
author2 Jiménez-Escobar, A.
Martín-Gago, José A.
Rogero, Celia
Atienza, C.
Puertas, S.
Sobrado, Jesús Manuel
Torres-Redondo, Josefina
author2_role author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Ministerio de Ciencia y Tecnología (España)
Ministerio de Ciencia e Innovación (España)
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv ISM: clouds
ISM: molecules
Molecular processes
Methods: laboratory
Infrared: ISM
Techniques: spectroscopic
topic ISM: clouds
ISM: molecules
Molecular processes
Methods: laboratory
Infrared: ISM
Techniques: spectroscopic
description [Aims]: We present the novel InterStellar Astrochemistry Chamber (ISAC), designed for studying solids (ice mantles, organics, and silicates) in interstellar and circumstellar environments: characterizing their physico-chemical properties and monitoring their evolution as caused by (i) vacuum-UV irradiation; (ii) cosmic ray irradiation; and (iii) thermal processing. Experimental study of thermal and photodesorption of the CO ice reported here simulates the freeze-out and desorption of CO on grains, providing new information on these processes. [Methods]: ISAC is an UHV set-up, with base pressure down to P = 2.5 × 10-11 mbar, where an ice layer is deposited at 7 K and can be UV-irradiated. The evolution of the solid sample was monitored by in situ transmittance FTIR spectroscopy, while the volatile species were monitored by QMS. [Results]: The UHV conditions of ISAC allow experiments under extremely clean conditions. Transmittance FTIR spectroscopy coupled to QMS proved to be ideal for in situ monitoring of ice processes that include radiation and thermal annealing. Thermal desorption of CO starting at 15 K, induced by the release of H2 from the CO ice, was observed. We measured the photodesorption yield of CO ice per incident photon at 7, 8, and 15 K, respectively yielding 6.4 ± 0.5 × 10-2, 5.4 ± 0.5 × 10-2, and 3.5 ± 0.5 × 10-2 CO molecules photon (7.3–10.5 eV)-1. Our value of the photodesorption yield of CO ice at 15 K is about one order of magnitude higher than the previous estimate. We confirmed that the photodesorption yield is constant during irradiation and independent of the ice thickness. Only below ~ 5 monolayers ice thickness the photodesorption rate decreases, which suggests that only the UV photons absorbed in the top 5 monolayers led to photodesorption. The measured CO photodesorption quantum yield at 7 K per absorbed photon in the top 5 monolayers is 3.4 molecules photon-1. [Conclusions]: Experimental values were used as input for a simple model of a quiescent cloud interior. Photodesorption seems to explain the observations of CO in the gas phase for densities below 3–7  × 104 cm-3. For the same density of a cloud, 3 × 104 cm-3, thermal desorption of CO is not triggered until T = 14.5 K. This has important implications for CO ice mantle build up in dark clouds.
publishDate 2010
dc.date.none.fl_str_mv 2010
2024
2024
2024
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/344271
url http://hdl.handle.net/10261/344271
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv #PLACEHOLDER_PARENT_METADATA_VALUE#
info:eu-repo/grantAgreement/MICINN//AYA2008-06374
https://doi.org/10.1051/0004-6361/200912462

dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
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