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Article: Optically thick radio cores of narrow-waist bipolar nebulae

TitleOptically thick radio cores of narrow-waist bipolar nebulae
Authors
KeywordsPlanetary nebulae: general
Radio continuum: stars
Stars: AGB and post-AGB
Stars: evolution
Stars: mass loss
Stars: winds, outflows
Issue Date2007
PublisherInstitute of Physics Publishing, Inc. The Journal's web site is located at http://iopscience.iop.org/0004-637X/
Citation
Astrophysical Journal, 2007, v. 665 n. 1 PART 1, p. 341-354 How to Cite?
AbstractWe report our search for optically thick radio cores in 16 narrow-waist bipolar nebulae. Optically thick cores are a characteristic signature of collimated ionized winds. Eleven northern nebulae were observed with the Very Large Array (VLA) at 1.3 and 0.7 cm, and five southern nebulae were observed with the Australia Telescope Compact Array (ATCA) at 6 and 3.6 cm. Two northern objects, 19W32 and M1-91, and three southern objects, He 2-25, He 2-84, and Mz 3, were found to exhibit a compact radio core with a rising spectrum consistent with an ionized jet. Such jets have been seen in M2-9 and may be responsible for shaping bipolar structure in planetary nebulae. © 2007. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/80629
ISSN
2021 Impact Factor: 5.521
2020 SCImago Journal Rankings: 2.376
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorLee, THen_HK
dc.contributor.authorLim, Jen_HK
dc.contributor.authorKwok, Sen_HK
dc.date.accessioned2010-09-06T08:08:33Z-
dc.date.available2010-09-06T08:08:33Z-
dc.date.issued2007en_HK
dc.identifier.citationAstrophysical Journal, 2007, v. 665 n. 1 PART 1, p. 341-354en_HK
dc.identifier.issn0004-637Xen_HK
dc.identifier.urihttp://hdl.handle.net/10722/80629-
dc.description.abstractWe report our search for optically thick radio cores in 16 narrow-waist bipolar nebulae. Optically thick cores are a characteristic signature of collimated ionized winds. Eleven northern nebulae were observed with the Very Large Array (VLA) at 1.3 and 0.7 cm, and five southern nebulae were observed with the Australia Telescope Compact Array (ATCA) at 6 and 3.6 cm. Two northern objects, 19W32 and M1-91, and three southern objects, He 2-25, He 2-84, and Mz 3, were found to exhibit a compact radio core with a rising spectrum consistent with an ionized jet. Such jets have been seen in M2-9 and may be responsible for shaping bipolar structure in planetary nebulae. © 2007. The American Astronomical Society. All rights reserved.en_HK
dc.languageengen_HK
dc.publisherInstitute of Physics Publishing, Inc. The Journal's web site is located at http://iopscience.iop.org/0004-637X/en_HK
dc.relation.ispartofAstrophysical Journalen_HK
dc.rightsThe Astrophysical Journal. Copyright © University of Chicago Press.en_HK
dc.subjectPlanetary nebulae: generalen_HK
dc.subjectRadio continuum: starsen_HK
dc.subjectStars: AGB and post-AGBen_HK
dc.subjectStars: evolutionen_HK
dc.subjectStars: mass lossen_HK
dc.subjectStars: winds, outflowsen_HK
dc.titleOptically thick radio cores of narrow-waist bipolar nebulaeen_HK
dc.typeArticleen_HK
dc.identifier.openurlhttp://library.hku.hk:4550/resserv?sid=HKU:IR&issn=0004-637X&volume=665&spage=341&epage=354&date=2007&atitle=Optically+Thick+Radio+Cores+of+Narrow-Waist+Bipolar+Nebulaeen_HK
dc.identifier.emailLim, J: jjlim@hku.hken_HK
dc.identifier.emailKwok, S: deannote@hku.hken_HK
dc.identifier.authorityLim, J=rp00745en_HK
dc.identifier.authorityKwok, S=rp00716en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1086/519270en_HK
dc.identifier.scopuseid_2-s2.0-34548299942en_HK
dc.identifier.hkuros133753en_HK
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-34548299942&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume665en_HK
dc.identifier.issue1 PART 1en_HK
dc.identifier.spage341en_HK
dc.identifier.epage354en_HK
dc.identifier.isiWOS:000248675700025-
dc.publisher.placeUnited Statesen_HK
dc.identifier.scopusauthoridLee, TH=37027800000en_HK
dc.identifier.scopusauthoridLim, J=7403453870en_HK
dc.identifier.scopusauthoridKwok, S=22980498300en_HK
dc.identifier.issnl0004-637X-

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