Photometric observations of pre-main sequence objects.

Details Photometric observations of pre-main sequence objects. Photometric observations of pre-main sequence objects.

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26as..113..473f&link_type=abstract

Astronomy and Astrophysics Supplement, v.113, p.473

Astronomy and Astrophysics

Astrophysics

6

Stars: Variable, Stars: Pre-Main Sequence

Scientific paper

We present the observational data of a photometric monitoring of 24 pre-main sequence objects: T Tauri stars, Ae/Be Herbig stars and some unclassified objects. Observations were carried out from July 1988 to August 1992, using the UBV(RI)_c_ system. Variability with time scales from days to years and amplitudes in the V band larger than 0.1mag is found for a part of this sample. The analysis of the possible causes of this variability are discussed in separate papers (Fernandez & Eiroa 1995a, b).

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