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dc.contributor.authorGiammanco, C.
dc.contributor.authorSale, S.E.
dc.contributor.authorCorradi, R.L.M.
dc.contributor.authorBarlow, M.J.
dc.contributor.authorViironen, K.
dc.contributor.authorSabin, L.
dc.contributor.authorSantander-Garcia, M.
dc.contributor.authorFrew, D.J.
dc.contributor.authorGreimel, R.
dc.contributor.authorMiszalski, B.
dc.contributor.authorPhillipps, S.
dc.contributor.authorZijlstra, A.A.
dc.contributor.authorMampaso, A.
dc.contributor.authorDrew, J.E.
dc.contributor.authorParker, Q.A.
dc.contributor.authorNapiwotzki, R.
dc.date.accessioned2011-01-17T11:24:13Z
dc.date.available2011-01-17T11:24:13Z
dc.date.issued2011
dc.identifier.citationGiammanco , C , Sale , S E , Corradi , R L M , Barlow , M J , Viironen , K , Sabin , L , Santander-Garcia , M , Frew , D J , Greimel , R , Miszalski , B , Phillipps , S , Zijlstra , A A , Mampaso , A , Drew , J E , Parker , Q A & Napiwotzki , R 2011 , ' IPHAS extinction distances to planetary nebulae ' Astronomy and Astrophysics , vol. 525 . https://doi.org/10.1051/0004-6361/201014464
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 182251
dc.identifier.otherPURE UUID: 340e08c7-4c73-4bf1-a4d2-b7a0f919b11f
dc.identifier.otherdspace: 2299/5154
dc.identifier.otherScopus: 78649759172
dc.identifier.urihttp://hdl.handle.net/2299/5154
dc.descriptionOriginal article can be found at: http://www.aanda.org Copyright European Southern Observatory
dc.description.abstractAims. The determination of reliable distances to planetary nebulae (PNe) is a major difficulty in the study of this class of objects in the Galaxy. The availability of new photometric surveys such as IPHAS (the INT/WFC photometric Hα survey of the northern Galactic plane) covering large portions of the sky provide an opportunity to apply the so-called extinction method to determine the distances of a large number of objects. Methods. The technique is applied to a sample of 137 PNe located between –5 and 5 degrees in Galactic latitude, and between 29.52 and 215.49 degrees in longitude. The characteristics of the distance-extinction method and the main sources of errors are carefully discussed. Results. The data on the extinction of the PNe available in the literature, complemented by new observations, allow us to determine extinction distances for 70 PNe. A comparison with statistical distance scales from different authors is presented.en
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.subjectCatalogs
dc.subjectplanetary nebulae
dc.titleIPHAS extinction distances to planetary nebulaeen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201014464
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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