A search for rapid variability in T Tauri stars

Details A search for rapid variability in T Tauri stars A search for rapid variability in T Tauri stars

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.282..167s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 282, Issue 1, pp. 167-174.

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6

Accretion, Accretion Discs, Stars: Formation, Stars: Pre-Main-Sequence, Stars: Variable: Other

Scientific paper

We have obtained high-time-resolution CCD photometry of four classical T Tauri stars, and have conducted a search for rapid photometric variability with these data. Any real variations on time-scales of tens of minutes to hours are shown to be typically at most of order 0.01 mag for all four variables. The lack of flickering on short time-scales is used to place constraints on the lumpiness of the assumed accretion flow in magnetically funnelled accretion models.

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