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Conference Paper: Planetary nebulae detected in the Spitzer Space Telescope GLIMPSE 3D Legacy Survey
Title | Planetary nebulae detected in the Spitzer Space Telescope GLIMPSE 3D Legacy Survey |
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Authors | |
Keywords | Infrared: ISM Planetary nebulae: general Planetary nebulae: individual (m 1-41) Stars: AGB and post-AGB |
Issue Date | 2011 |
Publisher | Cambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU |
Citation | The IAU Symposium No. 283: 'Planetary Nebulae: an Eye to the Future', Puerto de la Cruz, Tenerife, Spain, 25-29 July 2011. In International Astronomical Union Proceedings, 2011, v. 7 n. S283, p. 528-529 How to Cite? |
Abstract | Due to interstellar extinction, optical census of Galactic planetary nebulae (PNs) is highly incomplete, and some compact H ii regions might have been mis-classified as PNs. The problem is particularly severe in the Galactic plane where the extinction in the optical is significant and hampers the detections of PNs. Unlike optical observations, infrared (IR) observations are hardly affected by interstellar extinction, and provide a good opportunity to study highly obscured PNs. In this study, we use the data from the Spitzer Legacy Infrared Mid-Plane Survey Extraordinaire 3D (GLIMPSE 3D) to investigate the mid-infrared (MIR) properties of PNs and PN candidates. © 2012 International Astronomical Union. |
Persistent Identifier | http://hdl.handle.net/10722/165695 |
ISSN | 2023 SCImago Journal Rankings: 0.121 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Zhang, Y | en_US |
dc.contributor.author | Kwok, S | en_US |
dc.contributor.author | Hsia, C | en_US |
dc.contributor.author | Nakashima, J | en_US |
dc.contributor.author | Koning, N | en_US |
dc.date.accessioned | 2012-09-20T08:22:13Z | - |
dc.date.available | 2012-09-20T08:22:13Z | - |
dc.date.issued | 2011 | en_US |
dc.identifier.citation | The IAU Symposium No. 283: 'Planetary Nebulae: an Eye to the Future', Puerto de la Cruz, Tenerife, Spain, 25-29 July 2011. In International Astronomical Union Proceedings, 2011, v. 7 n. S283, p. 528-529 | en_US |
dc.identifier.issn | 1743-9213 | - |
dc.identifier.uri | http://hdl.handle.net/10722/165695 | - |
dc.description.abstract | Due to interstellar extinction, optical census of Galactic planetary nebulae (PNs) is highly incomplete, and some compact H ii regions might have been mis-classified as PNs. The problem is particularly severe in the Galactic plane where the extinction in the optical is significant and hampers the detections of PNs. Unlike optical observations, infrared (IR) observations are hardly affected by interstellar extinction, and provide a good opportunity to study highly obscured PNs. In this study, we use the data from the Spitzer Legacy Infrared Mid-Plane Survey Extraordinaire 3D (GLIMPSE 3D) to investigate the mid-infrared (MIR) properties of PNs and PN candidates. © 2012 International Astronomical Union. | - |
dc.language | eng | en_US |
dc.publisher | Cambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU | - |
dc.relation.ispartof | International Astronomical Union Proceedings | en_US |
dc.rights | International Astronomical Union Proceedings. Copyright © Cambridge University Press. | - |
dc.subject | Infrared: ISM | - |
dc.subject | Planetary nebulae: general | - |
dc.subject | Planetary nebulae: individual (m 1-41) | - |
dc.subject | Stars: AGB and post-AGB | - |
dc.title | Planetary nebulae detected in the Spitzer Space Telescope GLIMPSE 3D Legacy Survey | en_US |
dc.type | Conference_Paper | en_US |
dc.identifier.email | Zhang, Y: zhangy96@hku.hk | en_US |
dc.identifier.email | Kwok, S: deannote@hku.hk | en_US |
dc.identifier.email | Hsia, C: xiazh@hku.hk | en_US |
dc.identifier.email | Nakashima, J: junichi@hku.hk | en_US |
dc.identifier.email | Koning, N: nkoning@iras.ucalgary.ca | - |
dc.identifier.authority | Zhang, Y=rp00841 | en_US |
dc.identifier.authority | Kwok, S=rp00716 | en_US |
dc.identifier.authority | Hsia, C=rp00706 | en_US |
dc.identifier.authority | Nakashima, J=rp00764 | en_US |
dc.description.nature | published_or_final_version | - |
dc.identifier.doi | 10.1017/S1743921312012264 | - |
dc.identifier.scopus | eid_2-s2.0-84865772755 | - |
dc.identifier.hkuros | 209391 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-84865772755&selection=ref&src=s&origin=recordpage | - |
dc.identifier.volume | 7 | - |
dc.identifier.issue | S283 | - |
dc.identifier.spage | 528 | - |
dc.identifier.epage | 529 | - |
dc.identifier.isi | WOS:000309944800167 | - |
dc.publisher.place | United Kingdom | - |
dc.description.other | The IAU Symposium No. 283: 'Planetary Nebulae: an Eye to the Future', Puerto de la Cruz, Tenerife, Spain, 25-29 July 2011. In International Astronomical Union Proceedings, 2011, v. 7 n. S283, p. 528-529 | - |
dc.identifier.scopusauthorid | Zhang, Y=23768446500 | - |
dc.identifier.scopusauthorid | Kwok, S=22980498300 | - |
dc.identifier.scopusauthorid | Hsia, CH=14058287100 | - |
dc.identifier.scopusauthorid | Nakashima, JI=35485342300 | - |
dc.identifier.scopusauthorid | Koning, N=15520613500 | - |
dc.identifier.issnl | 1743-9213 | - |