==================================================================== The Galactic Microquasar V4641 Sgr resumed its activity! ==================================================================== This Galactic microquasar (see the most recent AstroAlert issues) had become rather inactive after reaching its peak around May 24. However, the object has apparently "turned on" again since June 2. The report based on June 4 observations (Makoto Uemura, Kyoto University) follows: The light curve on June 4 taken at Ouda shows a large (amplitude=1.2mag) hump and many 0.2mag-small flares. The large hump has a peak at about June 4.65UT and a duration of ~3 hr. The small flares looks have a weak, but characteristic periodicity (50-100s). After the object experienced the hump, it returned at quiescent level. Follow-up observations are encouraged since amplitudes of modulations seem to become larger with time. Comparing these data with May 31-June 1 observations reported by Gianluca Masi and Franco Mallia at Campo Catino Astronomical Observatory, it has become evident that the source has resumed its activity. Please keep in mind that the huge 1999 September event was preceded month-long activity phase (sometimes looking interrupted by inactive phases). There may be a coming major flare-up. Please continue observing the object as intensively as you can! We have put on the VSNET webpage a new light curve drawn from the June 4 observation. The amplitude of the variation surpassed that on May 24. You can see the activity the object showed only half a day ago! http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Xray/v4641sgr02.html Regards, Taichi Kato VSNET Collaboration team ---------------------------------------------------------------------------- VSNET (Variable Star Network) is an international variable star observing network, covering various areas of novae, supernovae, cataclysmic variables (CVs), X-ray transients, and other classical eruptive, pulsating, and eclipsing variables. VSNET is one of invited contributing organizations to the SkyPub AstroAlert system. VSNET Home Page: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/ CCD observations of such targets are a relatively easy task for a 20-40cm telescope; simply take as many CCD frames (with exposure times 10-30 sec) as possible, spanning several hours per night. The only requirements are the weather and your patience! If you need more help on the observing technique, please feel free to ask on the vsnet-campaign list. We would sincerely appreciate volunteers who would join the VSNET Collaboration team to study the wonders of these exotic variable stars. To join the VSNET campaign collaborative list, send an e-mail to vsnet-adm@kusastro.kyoto-u.ac.jp (VSNET administrator) with a line "SUBSCRIBE vsnet-campaign." or your comment to join the collaboration team. ----------------------------------------------------------------------------