1978 photometry of V711 Tauri=HR 1099 - During the radio outburst

Abstract

We present differential magnitudes in V of the UB V system obtained at seven different observatories during 16 nights in February and March 1978, coincident with the large radio outburst, and compare them with the preoutburst light curve. The wave migrated from 0(min)= .67 to 0 .74 but did not change significantly in amplitude or shape. The overall brightness level did not change by more than Om.005.

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