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Article: IPHAS extinction distances to planetary nebulae

TitleIPHAS extinction distances to planetary nebulae
Authors
Keywordscatalogs
planetary nebulae: general
Issue Date2010
Citation
Astronomy and Astrophysics, 2010, v. 525, n. 3 How to Cite?
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. © 2010 ESO.
Persistent Identifierhttp://hdl.handle.net/10722/208915
ISSN
2014 Impact Factor: 4.378
2015 SCImago Journal Rankings: 2.446

 

DC FieldValueLanguage
dc.contributor.authorGiammanco, Corrado-
dc.contributor.authorSale, Stuart E.-
dc.contributor.authorCorradi, Romano L M-
dc.contributor.authorBarlow, Michael J.-
dc.contributor.authorViironen, Kerttu-
dc.contributor.authorSabin, Laurence-
dc.contributor.authorSantander-Garćia, Miguel-
dc.contributor.authorFrew, David J.-
dc.contributor.authorGreimel, Robert-
dc.contributor.authorMiszalski, Brent-
dc.contributor.authorPhillipps, Steven-
dc.contributor.authorZijlstra, Albert A.-
dc.contributor.authorMampaso, Antonio-
dc.contributor.authorDrew, Janet E.-
dc.contributor.authorParker, Quentin A.-
dc.contributor.authorNapiwotzki, Ralf-
dc.date.accessioned2015-03-23T02:02:11Z-
dc.date.available2015-03-23T02:02:11Z-
dc.date.issued2010-
dc.identifier.citationAstronomy and Astrophysics, 2010, v. 525, n. 3-
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/10722/208915-
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. © 2010 ESO.-
dc.languageeng-
dc.relation.ispartofAstronomy and Astrophysics-
dc.subjectcatalogs-
dc.subjectplanetary nebulae: general-
dc.titleIPHAS extinction distances to planetary nebulae-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1051/0004-6361/201014464-
dc.identifier.scopuseid_2-s2.0-78649759172-
dc.identifier.volume525-
dc.identifier.issue3-
dc.identifier.eissn1432-0746-

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