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Article: Emission-line objects in the Large Magellanic Cloud. Observations obtained with the FLAIR system

TitleEmission-line objects in the Large Magellanic Cloud. Observations obtained with the FLAIR system
Authors
Issue Date1-Jun-1992
PublisherEDP Sciences
Citation
Astronomy and Astrophysics Supplement Series, 1992, v. 93, n. 3, p. 495-507 How to Cite?
AbstractThe FLAIR multi-object, fibre-coupled, spectroscopy system on the UK Schmidt Telescope has been used to observe a miscellany of emission-line objects in the Large Magellanic Cloud. The observations have been used to demonstrate the system's ability to provide quantitative measurements of emission-line objects. A comparison is made with published data where possible, and new classifications and measurements are presented.
Persistent Identifierhttp://hdl.handle.net/10722/343588
ISSN
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorMorganl, D-
dc.contributor.authorWatson, F-
dc.contributor.authorParker, Q-
dc.date.accessioned2024-05-24T04:12:15Z-
dc.date.available2024-05-24T04:12:15Z-
dc.date.issued1992-06-01-
dc.identifier.citationAstronomy and Astrophysics Supplement Series, 1992, v. 93, n. 3, p. 495-507-
dc.identifier.issn0365-0138-
dc.identifier.urihttp://hdl.handle.net/10722/343588-
dc.description.abstractThe FLAIR multi-object, fibre-coupled, spectroscopy system on the UK Schmidt Telescope has been used to observe a miscellany of emission-line objects in the Large Magellanic Cloud. The observations have been used to demonstrate the system's ability to provide quantitative measurements of emission-line objects. A comparison is made with published data where possible, and new classifications and measurements are presented.-
dc.languageeng-
dc.publisherEDP Sciences-
dc.relation.ispartofAstronomy and Astrophysics Supplement Series-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.titleEmission-line objects in the Large Magellanic Cloud. Observations obtained with the FLAIR system-
dc.typeArticle-
dc.identifier.volume93-
dc.identifier.issue3-
dc.identifier.spage495-
dc.identifier.epage507-
dc.identifier.eissn1286-4846-
dc.identifier.isiWOS:A1992HW16800008-
dc.publisher.placeLES ULIS CEDEX-
dc.identifier.issnl0365-0138-

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