Photographic photometry of Magellanic Cloud cepheids

Photographic (B,V) light curves of 213 LMC and 180 SMC cepheids (and W Virginis stars) have been obtained and the relevant light-curve parameters derived. Comparison of this work with stars in common with photoelectric data indicate that the <V> and (<B> - <V>) magnitudes differ from their photoelectric counterparts by ±0ᵐ.09 and ±0ᵐ.12 respectively for the fainter cepheids (log P <0.8) and by ±0ᵐ.06 and ±0ᵐ.07 respectively for the brighter cepheids (log P >0.8).

Grantor dc:publisher.institution

Department of Astronomy

Year dc:date.issued

1980

Author dc:creator

• Martin, William Longmate

Advisor dc:contributor.advisor

• Warner, Brian

Language dc:language.iso

eng

Handle dc:identifier.uri

http://hdl.handle.net/11427/17895

OAI identifier oai:identifier

oai:open.uct.ac.za:11427/17895