J/MNRAS/368/1392     Flares of the close binary FL Vir    (Pettersen+, 2006)

Flare variability in the close binary FL Vir. Pettersen B.R. <Mon. Not. R. Astron. Soc., 368, 1392-1394 (2006)> =2006MNRAS.368.1392P 2006MNRAS.368.1392P
ADC_Keywords: Stars, flare ; Stars, double and multiple Keywords: techniques: photometric - binaries: close - stars: flare Abstract: The results of U-filter flare monitoring of the binary flare star FL Vir = Wolf 424 is presented. 57 flares with energies between 2x1028 and 2x1031erg were recorded in 20h of observation. The properties of flare occurrence and flare time-scales are analysed, and the flare activity level in 1980 April is determined to be Lf(U)=8.0x1026erg/s. This is larger than previously published results and may indicate a variation in the flare activity level on a time-scale of years. An analysis of existing data indicates that the flare activity level correlates with the relative orbital positions of the stars. Description: FL Vir = Wolf 424 = Gliese 473 AB was observed on seven nights in 1980 April with the 2.1-m Struve reflector at McDonald Observatory. A computer-controlled high-speed photometer was used to collect data through eight filters. Here, we analyse only the U-filter data. Objects: -------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------- 12 33 17.5 +09 01 14 FL Vir = Wolf 424 -------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 58 98 U-filter flare characteristics for FL Vir -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Seq Flare number 3 A1 --- m_Seq Multiplicity index on Flare 5- 14 A10 "YYYY/MM/DD" Date UT Date of the event 16- 23 A8 "h:m:s" Time Time of the maximum flare (hh:mm:ss) 25 A1 --- l_trise Limit flag on trise 26- 27 I2 s trise ? Flare rise time 29 A1 --- l_t0.5 Limit flag on t0.5 30- 33 I4 s t0.5 ? Decay time 35 A1 --- l_tdur Limit flag on tdur 36- 39 I4 s tdur ? Duration time 41- 45 F5.2 --- Ampl Flare amplitude 48- 51 F4.2 --- Noise Noise (sigma/I0) 53 A1 --- l_logEu Limit flag on logEu 54- 58 F5.2 [10-7W] logEu ? Cumulative energy of flare (1) -------------------------------------------------------------------------------- Note (1): logEu=0.98log(N/T)+26.43 where N is the number of flare and T is the observing time in seconds. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 18-Oct-2006
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