A new flare star member candidate in the Pleiades cluster

作者：Moualla M^*; Schmidt T O B; Neuhaueser R; Hambaryan V V; Errmann R; Trepl L; Broeg Ch; Eisenbeiss T; Mugrauer M; Marka C; Adam C; Ginski C; Pribulla T; Raetz S; Schmidt J; Berndt A; Maciejewski G; Roell T; Hohle M M; Tetzlaff N; Fiedler S; Baar S

来源：Astronomische Nachrichten, 2011, 332(7): 661-667.

DOI：10.1002/asna.201111580

• open clusters and associations: individual (Pleiades)
• stars: flare
• stars: late-type
• stars: low-mass, brown dwarfs
• techniques: photometric

We present a new flare star, which was discovered during our survey on a selected field at the edge of the Pleiades cluster. The field was observed in the period 2007-2010 with three different CCD-cameras at the University Observatory Jena with telescopes from 25 to 90 cm. The flare duration is almost one hour with an amplitude in the R-band of about 1.08 mag. The location of the flare star in a color-magnitude diagram is consistent with age and distance of the Pleiades. In the optical PSF of the flare star there are two 2MASS objects (unresolved in most images in the optical Jena PSF), so it is not yet known which one of them is responsible for this flare. The BVRIJHK colors yield spectral types of M1 and M2 with extinction being A(V) = 0.231 +/- 0.024 mag and A(V) = 0.266 +/- 0.020 for those two stars, consistent with the Pleiades cluster.

• 出版日期2011-8