The variable stars of the young LMC cluster NGC 2164

Details The variable stars of the young LMC cluster NGC 2164 The variable stars of the young LMC cluster NGC 2164

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....105..146w&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 105, no. 1, p. 146-154.

Astronomy and Astrophysics

Astronomy

7

Early Stars, Magellanic Clouds, Star Clusters, Variable Stars, Astronomical Photometry, Cepheid Variables, Charge Coupled Devices

Scientific paper

The present search of the LMC cluster NGC 2164 for variable stars has uncovered one new member classical Cepheid variable with 3.772-day period; attention is also given to photometry for a previously unknown field overtone Cepheid variable with 3.4626-day period, and the 10.6878-day period HV 12078, which may be a member of the young NGC 2156 cluster. The clear separation of fundamental and overtone pulsators in the period-luminosity-color relation of known LMC cluster Cepheids establishes that the NGC 2164 member is a true overtone.

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