Rotational Variability in Pre-Main-Sequence Stars: TWA 6 in 2008

Details Rotational Variability in Pre-Main-Sequence Stars: TWA 6 in 2008 Rotational Variability in Pre-Main-Sequence Stars: TWA 6 in 2008

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ibvs.5989....1l&link_type=abstract

Information Bulletin on Variable Stars, 5989, 1.

Physics

Photometry

Scientific paper

Differential BVRI CCD photometry of the TW Hydrae association star TWA 6
obtained in 2008 shows the star to have a photometric amplitude a factor
of 2.5 lower than observed in 2001. We discuss this difference in terms
of a possible solar-type activity cycle.

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