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Conference Paper: Extending the RP survey to the outer LMC

TitleExtending the RP survey to the outer LMC
Authors
KeywordsMagellanic Clouds
surveys
statistics
planetary nebulae: general
Issue Date2011
Citation
Proceedings of the International Astronomical Union, 2011, v. 7, n. S283, p. 480-481 How to Cite?
AbstractWe are extending our search for faint PNe in the LMC to include the outer 56 deg 2 area not covered in the original UKST survey of the central 25deg 2 region. Candidate PNe have been selected using the Magellanic Cloud Emission Line Survey (MCELS) and the first round of observations has yielded 93 new LMC PNe while confirming the 102 previously known PNe in the outer LMC. We plan to continue our spectroscopic object identification program until we cover all our remaining candidates in the survey area. These observations, providing medium and high resolution spectra from λ3650Å to λ6900Å will additionally be used to measure fluxes for a series of research projects including luminosity functions, abundances and LMC kinematics. © 2012 International Astronomical Union.
Persistent Identifierhttp://hdl.handle.net/10722/208948
ISSN
2020 SCImago Journal Rankings: 0.124
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorReid, Warren A.-
dc.contributor.authorParker, Quentin A.-
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. 480-481-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/10722/208948-
dc.description.abstractWe are extending our search for faint PNe in the LMC to include the outer 56 deg 2 area not covered in the original UKST survey of the central 25deg 2 region. Candidate PNe have been selected using the Magellanic Cloud Emission Line Survey (MCELS) and the first round of observations has yielded 93 new LMC PNe while confirming the 102 previously known PNe in the outer LMC. We plan to continue our spectroscopic object identification program until we cover all our remaining candidates in the survey area. These observations, providing medium and high resolution spectra from λ3650Å to λ6900Å will additionally be used to measure fluxes for a series of research projects including luminosity functions, abundances and LMC kinematics. © 2012 International Astronomical Union.-
dc.languageeng-
dc.relation.ispartofProceedings of the International Astronomical Union-
dc.subjectMagellanic Clouds-
dc.subjectsurveys-
dc.subjectstatistics-
dc.subjectplanetary nebulae: general-
dc.titleExtending the RP survey to the outer LMC-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1017/S1743921312012021-
dc.identifier.scopuseid_2-s2.0-84865738985-
dc.identifier.volume7-
dc.identifier.issueS283-
dc.identifier.spage480-
dc.identifier.epage481-
dc.identifier.eissn1743-9221-
dc.identifier.isiWOS:000309944800143-
dc.identifier.issnl1743-9213-

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