Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasp..104.1144r&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 104, no. 682, p. 1144-1151.
Astronomy and Astrophysics
Astronomy
12
Brightness Distribution, Pre-Main Sequence Stars, Stellar Spectrophotometry, T Tauri Stars, Charge Coupled Devices, Stellar Luminosity
Scientific paper
T Tauri stars have long been known to undergo irregular variations in brightness. Extended monitoring of these pre-main-sequence, solar-type stars is important to understanding the sources of variations. Using an automated telescope at Leuschner Observatory, we have developed a procedure to acquire differential photometry of classical T Tau stars in Taurus and Auriga. It is almost fully automatic, dramatically reducing the time necessary to process the data. We achieved accuracy of 0.02 mag in eight fields containing target stars down to 13th magnitude. Although most of the T Tau stars did vary, we find possible, but not definitive, periods for several targets. The variations in general are complex, but often are correlated over a few days.
Basri Gibor
Pennypacker Carl
Perlmutter Saul
Richter Matthew
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