VLA Observations of Radio Variability of ER Vulpeculae in 1995

Abstract

VLA continuous monitoring of ER Vul during two 11.5 hour sessions in September 1995 in the radio continuum at 3.6 cm (X-band) showed a variation pattern similar to that observed in 1990 and 1991, but at a lower mean flux level. Simultaneous observations with the EUVE satellite in the 70 - 140 A band did not show any significant flaring variability of the star.

9 pages including 3 figures (inserted with psfig) and one table; submitted to PASP

Cited by in corpus (2)

• VLA multifrequency observations of RS CVn binaries
• Investigating Ca II emission in the RS CVn binary ER Vulpeculae using the Broadening Function Formalism