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Article: An optical-infrared study of the young multipolar planetary nebula NGC 6644

TitleAn optical-infrared study of the young multipolar planetary nebula NGC 6644
Authors
Hsia, CHKwok, SZhang, YKoning, NVolk, K
KeywordsISM: general
Planetary nebulae:individual (NGC 6644)
Stars:individual (AGB)
Issue Date2010
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 2010, v. 725 n. 1, p. 173-183 How to Cite?
DOI: http://dx.doi.org/10.1088/0004-637X/725/1/173
AbstractHigh-resolution Hubble Space Telescope imaging of the compact planetary nebula NGC 6644 has revealed two pairs of bipolar lobes and a central ring lying close to the plane of the sky. From mid-infrared imaging obtained with the Gemini Telescope, we have found a dust torus which is oriented nearly perpendicular to one pair of the lobes. We suggest that NGC 6644 is a multipolar nebula and construct a three-dimensional model that allows the visualization of the object from different lines of sight. These results suggest that NGC 6644 may have similar intrinsic structures as other multipolar nebulae and the phenomenon of multipolar nebulosity may be more common than previously believed. © 2010. The American Astronomical Society.
Persistent Identifierhttp://hdl.handle.net/10722/130529
ISSN
2041-8205
2021 Impact Factor: 8.811
2020 SCImago Journal Rankings: 3.639
ISI Accession Number ID
WOS:000284576700035
Funding AgencyGrant Number
NASANAS5-26555
Research Grants Council of the Hong Kong Special Administrative Region, ChinaHKU 7031/10P
Natural Sciences and Engineering Council of Canada
Alberta Ingenuity
Killam Trusts
NASA Office of Space ScienceNAG5-7584
Funding Information:

Some of the data presented in this paper were obtained from the Multimission Archive at the Space Telescope Science Institute (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NAG5-7584 and by other grants and contracts. Other parts of this work are based on observations made with the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the Particle Physics and Astronomy Research Council (United Kingdom), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), CNPq (Brazil), and CONICET (Argentina), and with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. This work was partially supported by the Research Grants Council of the Hong Kong Special Administrative Region, China (project no. HKU 7031/10P.). N.K. acknowledges support by the Natural Sciences and Engineering Council of Canada, Alberta Ingenuity, and the Killam Trusts.

References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorHsia, CHen_HK
dc.contributor.authorKwok, Sen_HK
dc.contributor.authorZhang, Yen_HK
dc.contributor.authorKoning, Nen_HK
dc.contributor.authorVolk, Ken_HK
dc.date.accessioned2010-12-23T08:55:20Z-
dc.date.available2010-12-23T08:55:20Z-
dc.date.issued2010en_HK
dc.identifier.citationAstrophysical Journal Letters, 2010, v. 725 n. 1, p. 173-183en_HK
dc.identifier.issn2041-8205en_HK
dc.identifier.urihttp://hdl.handle.net/10722/130529-
dc.description.abstractHigh-resolution Hubble Space Telescope imaging of the compact planetary nebula NGC 6644 has revealed two pairs of bipolar lobes and a central ring lying close to the plane of the sky. From mid-infrared imaging obtained with the Gemini Telescope, we have found a dust torus which is oriented nearly perpendicular to one pair of the lobes. We suggest that NGC 6644 is a multipolar nebula and construct a three-dimensional model that allows the visualization of the object from different lines of sight. These results suggest that NGC 6644 may have similar intrinsic structures as other multipolar nebulae and the phenomenon of multipolar nebulosity may be more common than previously believed. © 2010. The American Astronomical Society.en_HK
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_HK
dc.relation.ispartofAstrophysical Journal Lettersen_HK
dc.subjectISM: generalen_HK
dc.subjectPlanetary nebulae:individual (NGC 6644)en_HK
dc.subjectStars:individual (AGB)en_HK
dc.titleAn optical-infrared study of the young multipolar planetary nebula NGC 6644en_HK
dc.typeArticleen_HK
dc.identifier.emailHsia, CH: xiazh@hku.hken_HK
dc.identifier.emailKwok, S: deannote@hku.hken_HK
dc.identifier.emailZhang, Y: zhangy96@hku.hken_HK
dc.identifier.authorityHsia, CH=rp00706en_HK
dc.identifier.authorityKwok, S=rp00716en_HK
dc.identifier.authorityZhang, Y=rp00841en_HK
dc.description.naturepostprint-
dc.identifier.doi10.1088/0004-637X/725/1/173en_HK
dc.identifier.scopuseid_2-s2.0-78650131993en_HK
dc.identifier.hkuros183432en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-78650131993&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume725en_HK
dc.identifier.issue1en_HK
dc.identifier.spage173en_HK
dc.identifier.epage183en_HK
dc.identifier.isiWOS:000284576700035-
dc.publisher.placeUnited Kingdomen_HK
dc.identifier.scopusauthoridHsia, CH=14058287100en_HK
dc.identifier.scopusauthoridKwok, S=22980498300en_HK
dc.identifier.scopusauthoridZhang, Y=23768446500en_HK
dc.identifier.scopusauthoridKoning, N=15520613500en_HK
dc.identifier.scopusauthoridVolk, K=7006571965en_HK
dc.identifier.issnl2041-8205-

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