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Conference Paper: HCO + emission possibly related with a shielding mechanism that protects water molecules in the young PN K 3-35

TitleHCO + emission possibly related with a shielding mechanism that protects water molecules in the young PN K 3-35
Authors
Gómez, YTafoya, DAnglada, GLoinard, LTorrelles, JMMiranda, LFOsorio, MFrancoHernández, RNyman, LNakashima, JDeguchi, S
KeywordsPlanetary Nebula
Radio Lines: Molecules
Stars: Circumstellar Matter
Stars: Individual (K 3-35)
Issue Date2008
PublisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU
Citation
Proceedings Of The International Astronomical Union, 2008, v. 4 S251, p. 173-174 How to Cite?
DOI: http://dx.doi.org/10.1017/S1743921308021509
AbstractWater maser emission has been detected only toward three planetary nebulae (PNe). In particular, in K3-35, the first PN where water vapor maser emission was detected, the components are located in a torus-like structure with a radius of 85 AU and also at the surprisingly large distance of 5000 AU from the star, in the tips of the bipolar lobes. The existence of these water molecules in PNe is puzzling, probably related to some unknown mechanism shielding them against the ionizing radiation. We report the detection of HCO + (J = 1 0) emission toward K 3-35, that not only suggests that dense molecular gas (~10 5 cm 3) is present in this PN, but also that this kind of PN can enrich their surroundings with organic molecules. © 2008 International Astronomical Union.
Persistent Identifierhttp://hdl.handle.net/10722/176198
ISSN
1743-9213
2020 SCImago Journal Rankings: 0.124
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorGómez, Yen_US
dc.contributor.authorTafoya, Den_US
dc.contributor.authorAnglada, Gen_US
dc.contributor.authorLoinard, Len_US
dc.contributor.authorTorrelles, JMen_US
dc.contributor.authorMiranda, LFen_US
dc.contributor.authorOsorio, Men_US
dc.contributor.authorFrancoHernández, Ren_US
dc.contributor.authorNyman, Len_US
dc.contributor.authorNakashima, Jen_US
dc.contributor.authorDeguchi, Sen_US
dc.date.accessioned2012-11-26T09:06:48Z-
dc.date.available2012-11-26T09:06:48Z-
dc.date.issued2008en_US
dc.identifier.citationProceedings Of The International Astronomical Union, 2008, v. 4 S251, p. 173-174en_US
dc.identifier.issn1743-9213en_US
dc.identifier.urihttp://hdl.handle.net/10722/176198-
dc.description.abstractWater maser emission has been detected only toward three planetary nebulae (PNe). In particular, in K3-35, the first PN where water vapor maser emission was detected, the components are located in a torus-like structure with a radius of 85 AU and also at the surprisingly large distance of 5000 AU from the star, in the tips of the bipolar lobes. The existence of these water molecules in PNe is puzzling, probably related to some unknown mechanism shielding them against the ionizing radiation. We report the detection of HCO + (J = 1 0) emission toward K 3-35, that not only suggests that dense molecular gas (~10 5 cm 3) is present in this PN, but also that this kind of PN can enrich their surroundings with organic molecules. © 2008 International Astronomical Union.en_US
dc.languageengen_US
dc.publisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAUen_US
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.subjectPlanetary Nebulaen_US
dc.subjectRadio Lines: Moleculesen_US
dc.subjectStars: Circumstellar Matteren_US
dc.subjectStars: Individual (K 3-35)en_US
dc.titleHCO + emission possibly related with a shielding mechanism that protects water molecules in the young PN K 3-35en_US
dc.typeConference_Paperen_US
dc.identifier.emailNakashima, J: junichi@hku.hken_US
dc.identifier.authorityNakashima, J=rp00764en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1017/S1743921308021509en_US
dc.identifier.scopuseid_2-s2.0-53349096814en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-53349096814&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume4en_US
dc.identifier.issueS251en_US
dc.identifier.spage173en_US
dc.identifier.epage174en_US
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridGómez, Y=7003912682en_US
dc.identifier.scopusauthoridTafoya, D=15521388000en_US
dc.identifier.scopusauthoridAnglada, G=7003699718en_US
dc.identifier.scopusauthoridLoinard, L=6603796954en_US
dc.identifier.scopusauthoridTorrelles, JM=55411810400en_US
dc.identifier.scopusauthoridMiranda, LF=7101918957en_US
dc.identifier.scopusauthoridOsorio, M=7006394332en_US
dc.identifier.scopusauthoridFrancoHernández, R=15848564200en_US
dc.identifier.scopusauthoridNyman, L=7006064444en_US
dc.identifier.scopusauthoridNakashima, J=35485342300en_US
dc.identifier.scopusauthoridDeguchi, S=7006314159en_US
dc.identifier.issnl1743-9213-

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