Near-infrared time-series photometry of six fields in the young open cluster IC 2391

Details Near-infrared time-series photometry of six fields in the young open cluster IC 2391 Near-infrared time-series photometry of six fields in the young open cluster IC 2391

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006mnras.369..846k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 369, Issue 2, pp. 846-852.

Other

3

Stars: Low-Mass, Brown Dwarfs: Stars: Variables: Other, Brown Dwarfs, Stars: Variables: Other

Scientific paper

Fields containing targets of spectral types later than M5 were monitored in JHKs for about 7h each. None of the targets showed variability at levels exceeding 0.02 (or smaller, in some cases). Seven new variable stars were discovered serendipitously. The large number of measurements (more than 50) of each field allows the construction of accurate colour-magnitude and colour-colour diagrams. These could be used to identify a small number of candidate very cool objects.

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