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- Publisher Website: 10.1088/0004-637X/722/1/273
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Article: Detection of multiple bipolar flows in NGC 7027 with submillimeter array
Title | Detection of multiple bipolar flows in NGC 7027 with submillimeter array |
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Authors | |
Keywords | ISM: molecules Planetary nebulae: individual (NGC 7027) |
Issue Date | 2010 |
Publisher | Institute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205 |
Citation | Astrophysical Journal Letters, 2010, v. 722 n. 1, p. 273-280 How to Cite? |
Abstract | Highly collimated multiple bipolar flows are detected with a 3′′ resolution in the HCO+ (J = 3-2) and HCN (J = 3-2) lines in the young planetary nebula NGC 7027 with the Submillimeter Array. The HCO + and HCN flows coincide in location and velocity with compact and fast CO flows detected with ~6′′ resolutions with other millimeter arrays. The equatorial molecular torus of NGC 7027 is captured in HCO + emission in the present observations. The HCO + emission also closely follows the H 2 emission, indicating that the present observations probe the photon-dominated region of the molecular envelope of NGC 7027. © 2010. The American Astronomical Society. All rights reserved. |
Persistent Identifier | http://hdl.handle.net/10722/128494 |
ISSN | 2023 Impact Factor: 8.8 2023 SCImago Journal Rankings: 2.766 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
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dc.contributor.author | Huang, ZY | en_HK |
dc.contributor.author | Hasegawa, TI | en_HK |
dc.contributor.author | Trung, DV | en_HK |
dc.contributor.author | Kwok, S | en_HK |
dc.contributor.author | Muller, S | en_HK |
dc.contributor.author | Hirano, N | en_HK |
dc.contributor.author | Lim, J | en_HK |
dc.contributor.author | Mariappan, CM | en_HK |
dc.contributor.author | Lyo, A | en_HK |
dc.date.accessioned | 2010-10-31T14:31:34Z | - |
dc.date.available | 2010-10-31T14:31:34Z | - |
dc.date.issued | 2010 | en_HK |
dc.identifier.citation | Astrophysical Journal Letters, 2010, v. 722 n. 1, p. 273-280 | en_HK |
dc.identifier.issn | 2041-8205 | en_HK |
dc.identifier.uri | http://hdl.handle.net/10722/128494 | - |
dc.description.abstract | Highly collimated multiple bipolar flows are detected with a 3′′ resolution in the HCO+ (J = 3-2) and HCN (J = 3-2) lines in the young planetary nebula NGC 7027 with the Submillimeter Array. The HCO + and HCN flows coincide in location and velocity with compact and fast CO flows detected with ~6′′ resolutions with other millimeter arrays. The equatorial molecular torus of NGC 7027 is captured in HCO + emission in the present observations. The HCO + emission also closely follows the H 2 emission, indicating that the present observations probe the photon-dominated region of the molecular envelope of NGC 7027. © 2010. The American Astronomical Society. All rights reserved. | en_HK |
dc.language | eng | en_HK |
dc.publisher | Institute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205 | en_HK |
dc.relation.ispartof | Astrophysical Journal Letters | en_HK |
dc.subject | ISM: molecules | en_HK |
dc.subject | Planetary nebulae: individual (NGC 7027) | en_HK |
dc.title | Detection of multiple bipolar flows in NGC 7027 with submillimeter array | en_HK |
dc.type | Article | en_HK |
dc.identifier.openurl | http://library.hku.hk:4550/resserv?sid=HKU:IR&issn=0004-637X&volume=722&spage=273&epage=280&date=2010&atitle=Detection+of+Multiple+Bipolar+Flows+in+NGC+7027+with+Submillimeter+Array | en_HK |
dc.identifier.email | Kwok, S: deannote@hku.hk | en_HK |
dc.identifier.email | Lim, J: jjlim@hku.hk | en_HK |
dc.identifier.authority | Kwok, S=rp00716 | en_HK |
dc.identifier.authority | Lim, J=rp00745 | en_HK |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1088/0004-637X/722/1/273 | en_HK |
dc.identifier.scopus | eid_2-s2.0-78149342885 | en_HK |
dc.identifier.hkuros | 181416 | en_HK |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-78149342885&selection=ref&src=s&origin=recordpage | en_HK |
dc.identifier.volume | 722 | en_HK |
dc.identifier.issue | 1 | en_HK |
dc.identifier.spage | 273 | en_HK |
dc.identifier.epage | 280 | en_HK |
dc.identifier.isi | WOS:000282908900024 | - |
dc.publisher.place | United Kingdom | en_HK |
dc.identifier.scopusauthorid | Huang, ZY=36617339700 | en_HK |
dc.identifier.scopusauthorid | Hasegawa, TI=7404173711 | en_HK |
dc.identifier.scopusauthorid | Trung, DV=6701469660 | en_HK |
dc.identifier.scopusauthorid | Kwok, S=22980498300 | en_HK |
dc.identifier.scopusauthorid | Muller, S=15071043100 | en_HK |
dc.identifier.scopusauthorid | Hirano, N=35769189500 | en_HK |
dc.identifier.scopusauthorid | Lim, J=7403453870 | en_HK |
dc.identifier.scopusauthorid | Mariappan, CM=36617692300 | en_HK |
dc.identifier.scopusauthorid | Lyo, A=6508022172 | en_HK |
dc.identifier.issnl | 2041-8205 | - |