Photometry of 40 large magellanic cloud cepheids

dc.contributor.author	Tanvir, N. R.
dc.contributor.author	Boyle, A.
dc.date.accessioned	2018-08-24T08:26:31Z
dc.date.available	2018-08-24T08:26:31Z
dc.date.issued	1999-04-16
dc.identifier.citation	Tanvir, N. R. Boyle, A. (1999). Photometry of 40 large magellanic cloud cepheids. Monthly Notices of the Royal Astronomical Society 304 (4), 957-960
dc.identifier.issn	0035-8711,1365-2966
dc.identifier.uri	http://hdl.handle.net/10379/9928
dc.description.abstract	We present V and I-c CCD photometry for 40 Large Magellanic Cloud (LMC) Cepheids at 1 to 3 epochs. This represents a significant increase in the number of LMC Cepheids with I-band data, and, as we show, is a useful addition to the sample that can be used to calibrate the period-luminosity relations in these important bands.
dc.publisher	Oxford University Press (OUP)
dc.relation.ispartof	Monthly Notices of the Royal Astronomical Society
dc.rights	Attribution-NonCommercial-NoDerivs 3.0 Ireland
dc.rights.uri	https://creativecommons.org/licenses/by-nc-nd/3.0/ie/
dc.subject	cepheids
dc.subject	magellanic clouds
dc.subject	standard stars
dc.subject	celestial equator
dc.title	Photometry of 40 large magellanic cloud cepheids
dc.type	Article
dc.identifier.doi	10.1046/j.1365-8711.1999.02387.x
dc.local.publishedsource	https://academic.oup.com/mnras/article-pdf/304/4/957/3572977/304-4-957.pdf
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