Investigation of variable stars in the region of NGC 1854 in the Large Magellanic Cloud

Details Investigation of variable stars in the region of NGC 1854 in the Large Magellanic Cloud Investigation of variable stars in the region of NGC 1854 in the Large Magellanic Cloud

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..405k&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 405, translation of Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 11, p

Astronomy and Astrophysics

Astronomy

1

Interstellar Extinction, Light Curve, Magellanic Clouds, Star Clusters, Variable Stars, Astronomical Observatories, Astronomical Photography, Cepheid Variables, Milky Way Galaxy, Photographic Plates

Scientific paper

Light changes of 48 variable stars in a 0.9 x 0.9 deg field with the center at 05 h 10 m - 68.9 deg in the LMC cluster NGC 1854 are studied. Refined values of Cepheid periods are obtained, and possible changes when compared with the data of Payne-Gaposchkin (1970), obtained in the first half of the century, are identified. The calculated distance modulus of LMC m-M is 18.08 +/- 0.14 m if the period-luminosity relation of Kraft (1961) for Cepheids of the galaxy is applied.

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