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Conference Paper: New faint planetary nebulae from the DSS and SDSS

TitleNew faint planetary nebulae from the DSS and SDSS
Authors
Keywordssurveys
planetary nebulae: general
Issue Date2011
Citation
Proceedings of the International Astronomical Union, 2011, v. 7, n. S283, p. 414-415 How to Cite?
AbstractHaving surveyed ≈ 10% of the sky, we have identified more than 130 PN candidates by surveying multicolour Digitized Sky Survey (DSS), Sloan Digitized Sky Survey (SDSS), and combined [O III], Hα and [S II] images. In a first imaging and spectroscopy campaign, 51 objects were identified as true and probable PNe. This work presents an additional 17 probable or possible PNe identified since that study. The majority of these candidates are situated at Galactic latitudes |b| > 5°, with the exception of seven objects located closer to the Galactic plane. Using the techniques described here that do not require any new survey data, we anticipate that many more PNe are waiting to be found, perhaps as many as 90. © 2012 International Astronomical Union.
Persistent Identifierhttp://hdl.handle.net/10722/208945
ISSN
2015 SCImago Journal Rankings: 0.105

 

DC FieldValueLanguage
dc.contributor.authorKronberger, Matthias-
dc.contributor.authorJacoby, George H.-
dc.contributor.authorCiardullo, Robin-
dc.contributor.authorCrisp, Richard D.-
dc.contributor.authorDe Marco, Orsola-
dc.contributor.authorDouchin, Dimitri-
dc.contributor.authorFrew, David J.-
dc.contributor.authorHarmer, Dianne L.-
dc.contributor.authorHowell, Michael-
dc.contributor.authorHowell, Steve B.-
dc.contributor.authorParker, Quentin A.-
dc.contributor.authorPatchick, Dana-
dc.contributor.authorRector, Travis A.-
dc.contributor.authorRiddle, Dave-
dc.contributor.authorTeutsch, Philipp-
dc.date.accessioned2015-03-23T02:02:19Z-
dc.date.available2015-03-23T02:02:19Z-
dc.date.issued2011-
dc.identifier.citationProceedings of the International Astronomical Union, 2011, v. 7, n. S283, p. 414-415-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/10722/208945-
dc.description.abstractHaving surveyed ≈ 10% of the sky, we have identified more than 130 PN candidates by surveying multicolour Digitized Sky Survey (DSS), Sloan Digitized Sky Survey (SDSS), and combined [O III], Hα and [S II] images. In a first imaging and spectroscopy campaign, 51 objects were identified as true and probable PNe. This work presents an additional 17 probable or possible PNe identified since that study. The majority of these candidates are situated at Galactic latitudes |b| > 5°, with the exception of seven objects located closer to the Galactic plane. Using the techniques described here that do not require any new survey data, we anticipate that many more PNe are waiting to be found, perhaps as many as 90. © 2012 International Astronomical Union.-
dc.languageeng-
dc.relation.ispartofProceedings of the International Astronomical Union-
dc.subjectsurveys-
dc.subjectplanetary nebulae: general-
dc.titleNew faint planetary nebulae from the DSS and SDSS-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1017/S1743921312011696-
dc.identifier.scopuseid_2-s2.0-84865716373-
dc.identifier.volume7-
dc.identifier.issueS283-
dc.identifier.spage414-
dc.identifier.epage415-
dc.identifier.eissn1743-9221-

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