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Article: A study of H2 emission in the bipolar proto-planetary nebula IRAS 17150-3224

TitleA study of H2 emission in the bipolar proto-planetary nebula IRAS 17150-3224
Authors
Hrivnak, BJKelly, DMSu, KYLKwok, SSahai, R
KeywordsCircumstellar Matter
Infrared: Stars
Planetary Nebulae: General Stars: Agb And Post-Agb
Stars: Mass Loss
Issue Date2006
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/0004-637X
Citation
The Astrophysical Journal, 2006, v. 650 n. 1 pt. 1, p. 237-245 How to Cite?
DOI: http://dx.doi.org/10.1086/506014
AbstractH 2 emission has been detected in the bipolar proto-planetaiy nebula IRAS 17150 - 3224 from the 1 -0 S(1), 1-0 S(0), and 2-1 S(1) transitions in the 2 μm region. Line ratios suggest that this emission is due to collisional excitation. High-resolution imaging with NICMOS on HSTshows that the emission comes from four regions: clumps near the ends of the lobes (the brightest region), the lobes in general, a particular region outside the northwest lobe, and a faint loop in the equatorial region. Spatially resolved high-resolution spectra at 2.12 μm reveal that the H 2 1-0 S(1) line has a velocity width of about 35 km s -1 in the lobes, consistent with C-type shocks. The emission from the clumps in the lobes appears to arise from the impact of a fast wind with the slower moving material in the AGB wind. © 2006. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/179709
ISSN
0004-637X
2023 Impact Factor: 4.8
2023 SCImago Journal Rankings: 1.905
ISI Accession Number ID
WOS:000241193400020
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorHrivnak, BJen_US
dc.contributor.authorKelly, DMen_US
dc.contributor.authorSu, KYLen_US
dc.contributor.authorKwok, Sen_US
dc.contributor.authorSahai, Ren_US
dc.date.accessioned2012-12-19T10:03:10Z-
dc.date.available2012-12-19T10:03:10Z-
dc.date.issued2006en_US
dc.identifier.citationThe Astrophysical Journal, 2006, v. 650 n. 1 pt. 1, p. 237-245en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/179709-
dc.description.abstractH 2 emission has been detected in the bipolar proto-planetaiy nebula IRAS 17150 - 3224 from the 1 -0 S(1), 1-0 S(0), and 2-1 S(1) transitions in the 2 μm region. Line ratios suggest that this emission is due to collisional excitation. High-resolution imaging with NICMOS on HSTshows that the emission comes from four regions: clumps near the ends of the lobes (the brightest region), the lobes in general, a particular region outside the northwest lobe, and a faint loop in the equatorial region. Spatially resolved high-resolution spectra at 2.12 μm reveal that the H 2 1-0 S(1) line has a velocity width of about 35 km s -1 in the lobes, consistent with C-type shocks. The emission from the clumps in the lobes appears to arise from the impact of a fast wind with the slower moving material in the AGB wind. © 2006. The American Astronomical Society. All rights reserved.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/0004-637Xen_US
dc.relation.ispartofThe Astrophysical Journalen_US
dc.rightsThe Astrophysical Journal. Copyright © University of Chicago Press.-
dc.subjectCircumstellar Matteren_US
dc.subjectInfrared: Starsen_US
dc.subjectPlanetary Nebulae: General Stars: Agb And Post-Agben_US
dc.subjectStars: Mass Lossen_US
dc.titleA study of H2 emission in the bipolar proto-planetary nebula IRAS 17150-3224en_US
dc.typeArticleen_US
dc.identifier.emailKwok, S: deannote@hku.hken_US
dc.identifier.authorityKwok, S=rp00716en_US
dc.description.naturepublished_or_final_versionen_US
dc.identifier.doi10.1086/506014en_US
dc.identifier.scopuseid_2-s2.0-37849187017en_US
dc.identifier.hkuros124998-
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-37849187017&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume650en_US
dc.identifier.issue1 pt. 1en_US
dc.identifier.spage237en_US
dc.identifier.epage245en_US
dc.identifier.isiWOS:000241193400020-
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridHrivnak, BJ=35613962100en_US
dc.identifier.scopusauthoridKelly, DM=13104011200en_US
dc.identifier.scopusauthoridSu, KYL=26326482200en_US
dc.identifier.scopusauthoridKwok, S=22980498300en_US
dc.identifier.scopusauthoridSahai, R=7004985042en_US
dc.identifier.issnl0004-637X-

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