VI light curves of LMC R CBr stars (Soszynski+, 2009)

Details VI light curves of LMC R CBr stars (Soszynski+, 2009) VI light curves of LMC R CBr stars (Soszynski+, 2009)

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat.120590335s&link_type=abstract

VizieR On-line Data Catalog: J/AcA/59/335. Originally published in: 2009AcA....59..335S

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Magellanic Clouds, Stars: Variable, Magnitudes

Scientific paper

We use the sample of carbon-rich long-period variables released in the previous part of this catalog to select objects with severe drops in luminosity, i.e., with the DY-Per-like light curves. DY Per stars are often related to R CrB variables. We detect at least 600 candidates for DY Per stars, mostly among dust enshrouded giants. We notice that our candidate DY Per stars form a continuity with other carbon-rich long-period variables, so it seems that DY Per stars do not constitute a separate group of variable stars.
(1 data file).

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