VI light curves of LMC long-period variables (Soszynski+, 2009)

Details VI light curves of LMC long-period variables (Soszynski+, 2009) VI light curves of LMC long-period variables (Soszynski+, 2009)

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat.120590239s&link_type=abstract

VizieR On-line Data Catalog: J/AcA/59/239. Originally published in: 2009AcA....59..239S

Physics

Magellanic Clouds, Stars: Variable, Magnitudes

Scientific paper

We describe the methods used for the identification and classification of LPVs. The distribution of I-band amplitudes for carbon-rich stars shows two maxima, corresponding to Miras and SRVs. Such a distinction between Miras and SRVs is not obvious for oxygen-rich stars. We notice additional period-luminosity sequence located between Wood's sequences C and C' and populated by SRVs.
(1 data file).

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