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By Zs. Kővári, F. Vilardell, I. Ribas, K. Vida, L. Van Driel-gesztelyi, C. Jordi and K. Oláh

Abstract

We present B and V light curves of a large stellar flare obtained with the Wide Field Camera at the Isaac Newton 2.5-m telescope (La Palma). The source object is a faint (mV = 21.38) foreground star in the field of the Andromeda galaxy, with its most probable spectral type being dM4. We provide an estimate of the total flare energy in the optical range an

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Year: 2007
OAI identifier: oai:CiteSeerX.psu:10.1.1.316.685
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