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Article: Radio-continuum detections of Galactic Planetary Nebulae - I. MASH PNe detected in large-scale radio surveys

TitleRadio-continuum detections of Galactic Planetary Nebulae - I. MASH PNe detected in large-scale radio surveys
Authors
KeywordsPlanetary nebulae: general
Astronomical data bases: miscellaneous
Radio continuum: ISM
Radiation mechanisms: thermal
Issue Date2011
Citation
Monthly Notices of the Royal Astronomical Society, 2011, v. 412, n. 1, p. 223-245 How to Cite?
AbstractWe present an updated and newly compiled radio-continuum data base for Macquarie/AAO/Strasbourg Hα (MASH) planetary nebulae (PNe) detected in the extant large-scale 'blind' radio-continuum surveys [NRAO VLA Sky Survey (NVSS), Sydney University Molonglo Sky Survey/Molonglo Galactic Plane Surveys (SUMSS/MGPS-2) and Parkes-MIT-NRAO (PMN)] and, for a small number of MASH PNe, observed and detected in targeted radio-continuum observations. We found radio counterparts for approximately 250 MASH PNe. In comparison with the percentage of previously known Galactic PNe detected in the NVSS and MGPS-2 radio-continuum surveys and according to their position on the flux density angular diameter and the radio brightness temperature evolutionary diagrams we conclude, unsurprisingly, that the MASH sample presents the radio-faint end of the known Galactic PNe population. Also, we present radio-continuum spectral properties of a small sub-sample of MASH PNe located in the strip between declinations -30° and -40°, that are detected in both the NVSS and MGPS-2 radio surveys. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.
Persistent Identifierhttp://hdl.handle.net/10722/208922
ISSN
2015 Impact Factor: 4.952
2015 SCImago Journal Rankings: 2.806

 

DC FieldValueLanguage
dc.contributor.authorBojičić, Ivan S.-
dc.contributor.authorParker, Quentin A.-
dc.contributor.authorFilipovíc, Miroslav D.-
dc.contributor.authorFrew, David J.-
dc.date.accessioned2015-03-23T02:02:12Z-
dc.date.available2015-03-23T02:02:12Z-
dc.date.issued2011-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2011, v. 412, n. 1, p. 223-245-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/208922-
dc.description.abstractWe present an updated and newly compiled radio-continuum data base for Macquarie/AAO/Strasbourg Hα (MASH) planetary nebulae (PNe) detected in the extant large-scale 'blind' radio-continuum surveys [NRAO VLA Sky Survey (NVSS), Sydney University Molonglo Sky Survey/Molonglo Galactic Plane Surveys (SUMSS/MGPS-2) and Parkes-MIT-NRAO (PMN)] and, for a small number of MASH PNe, observed and detected in targeted radio-continuum observations. We found radio counterparts for approximately 250 MASH PNe. In comparison with the percentage of previously known Galactic PNe detected in the NVSS and MGPS-2 radio-continuum surveys and according to their position on the flux density angular diameter and the radio brightness temperature evolutionary diagrams we conclude, unsurprisingly, that the MASH sample presents the radio-faint end of the known Galactic PNe population. Also, we present radio-continuum spectral properties of a small sub-sample of MASH PNe located in the strip between declinations -30° and -40°, that are detected in both the NVSS and MGPS-2 radio surveys. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.-
dc.languageeng-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
dc.subjectPlanetary nebulae: general-
dc.subjectAstronomical data bases: miscellaneous-
dc.subjectRadio continuum: ISM-
dc.subjectRadiation mechanisms: thermal-
dc.titleRadio-continuum detections of Galactic Planetary Nebulae - I. MASH PNe detected in large-scale radio surveys-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1111/j.1365-2966.2010.17900.x-
dc.identifier.scopuseid_2-s2.0-79952621142-
dc.identifier.volume412-
dc.identifier.issue1-
dc.identifier.spage223-
dc.identifier.epage245-
dc.identifier.eissn1365-2966-

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