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Article: Planetary nebulae detected in the spitzer space telescope glimpse II legacy survey
Title | Planetary nebulae detected in the spitzer space telescope glimpse II legacy survey | ||||||||||||||
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Authors | |||||||||||||||
Keywords | Infrared: ISM Planetary nebulae: general Stars: AGB and post-AGB | ||||||||||||||
Issue Date | 2009 | ||||||||||||||
Publisher | Institute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205 | ||||||||||||||
Citation | Astrophysical Journal Letters, 2009, v. 706 n. 1, p. 252-305 How to Cite? | ||||||||||||||
Abstract | We report the result of a search for the infrared counterparts of 37 planetary nebulae (PNs) and PN candidates in the Spitzer Galactic Legacy Infrared Mid-Plane Survey Extraordinaire II (GLIMPSE II) survey. The photometry and images of these PNs at 3.6, 4.5, 5.8, 8.0, and 24 μm, taken through the Infrared Array Camera (IRAC) and the Multiband Imaging Photometer for Spitzer (MIPS), are presented. Most of these nebulae are very red and compact in the IRAC bands, and are found to be bright and extended in the 24 μm band. The infrared morphology of these objects are compared with Hα images of the Macquarie-AAO-Strasbourg (MASH) and MASH II PNs. The implications for morphological difference in different wavelengths are discussed. The IRAC data allow us to differentiate between PNs and H II regions and be able to reject non-PNs from the optical catalog (e.g., PNG 352.1 - 00.0). Spectral energy distributions are constructed by combing the IRAC and MIPS data with existing near-, mid-, and far-IR photometry measurements. The anomalous colors of some objects allow us to infer the presence of aromatic emission bands. These multi-wavelength data provide useful insights into the nature of different nebular components contributing to the infrared emission of PNs. © 2009. The American Astronomical Society. All rights reserved. | ||||||||||||||
Persistent Identifier | http://hdl.handle.net/10722/90478 | ||||||||||||||
ISSN | 2023 Impact Factor: 8.8 2023 SCImago Journal Rankings: 2.766 | ||||||||||||||
ISI Accession Number ID |
Funding Information: We also thank Nico Koning for his help in data processing and Jun-ichi Nakashima for fruitful discussion. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA. This study used data products from the GLIMPSE and MIPSGAL Spitzer Space Telescope Legacy Programs. This publication also used the data products from the DENIS project, which has been partly funded by the SCIENCE and the HCM plans of the European Commission under grants CT920791 and CT940627, from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation, and from the Midcourse Space Experiment, which was funded by the Ballistic Missile Defense Organization with additional support from NASA Office of Space Science. This research has also made use of the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, and made use of the SIMBAD database, operated at CDS, Strasbourg, France. Support for this work was provided by the Research Grants Council of the Hong Kong under grants HKU7032/09P. | ||||||||||||||
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Zhang, Y | en_HK |
dc.contributor.author | Kwok, S | en_HK |
dc.date.accessioned | 2010-09-06T10:11:12Z | - |
dc.date.available | 2010-09-06T10:11:12Z | - |
dc.date.issued | 2009 | en_HK |
dc.identifier.citation | Astrophysical Journal Letters, 2009, v. 706 n. 1, p. 252-305 | en_HK |
dc.identifier.issn | 2041-8205 | en_HK |
dc.identifier.uri | http://hdl.handle.net/10722/90478 | - |
dc.description.abstract | We report the result of a search for the infrared counterparts of 37 planetary nebulae (PNs) and PN candidates in the Spitzer Galactic Legacy Infrared Mid-Plane Survey Extraordinaire II (GLIMPSE II) survey. The photometry and images of these PNs at 3.6, 4.5, 5.8, 8.0, and 24 μm, taken through the Infrared Array Camera (IRAC) and the Multiband Imaging Photometer for Spitzer (MIPS), are presented. Most of these nebulae are very red and compact in the IRAC bands, and are found to be bright and extended in the 24 μm band. The infrared morphology of these objects are compared with Hα images of the Macquarie-AAO-Strasbourg (MASH) and MASH II PNs. The implications for morphological difference in different wavelengths are discussed. The IRAC data allow us to differentiate between PNs and H II regions and be able to reject non-PNs from the optical catalog (e.g., PNG 352.1 - 00.0). Spectral energy distributions are constructed by combing the IRAC and MIPS data with existing near-, mid-, and far-IR photometry measurements. The anomalous colors of some objects allow us to infer the presence of aromatic emission bands. These multi-wavelength data provide useful insights into the nature of different nebular components contributing to the infrared emission of PNs. © 2009. 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.rights | The Astrophysical Journal. Copyright © Institute of Physics Publishing, Inc. | en_HK |
dc.subject | Infrared: ISM | en_HK |
dc.subject | Planetary nebulae: general | en_HK |
dc.subject | Stars: AGB and post-AGB | en_HK |
dc.title | Planetary nebulae detected in the spitzer space telescope glimpse II legacy survey | en_HK |
dc.type | Article | en_HK |
dc.identifier.openurl | http://library.hku.hk:4550/resserv?sid=HKU:IR&issn=0004-637X&volume=706&issue=1&spage=252&epage=305&date=2009&atitle=Planetary+nebulae+detected+in+the+spitzer+space+telescope+glimpse+II+legacy+survey | en_HK |
dc.identifier.email | Zhang, Y: zhangy96@hku.hk | en_HK |
dc.identifier.email | Kwok, S: deannote@hku.hk | en_HK |
dc.identifier.authority | Zhang, Y=rp00841 | en_HK |
dc.identifier.authority | Kwok, S=rp00716 | en_HK |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1088/0004-637X/706/1/252 | en_HK |
dc.identifier.scopus | eid_2-s2.0-70549090239 | en_HK |
dc.identifier.hkuros | 168227 | en_HK |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-70549090239&selection=ref&src=s&origin=recordpage | en_HK |
dc.identifier.volume | 706 | en_HK |
dc.identifier.issue | 1 | en_HK |
dc.identifier.spage | 252 | en_HK |
dc.identifier.epage | 305 | en_HK |
dc.identifier.eissn | 1538-4357 | - |
dc.identifier.isi | WOS:000271538900022 | - |
dc.publisher.place | United Kingdom | en_HK |
dc.identifier.scopusauthorid | Zhang, Y=23768446500 | en_HK |
dc.identifier.scopusauthorid | Kwok, S=22980498300 | en_HK |