Dear All, On July 14, 1997, ALEXIS detected a transient in Telescope 3B (186 Angstroms) which appeared to last approximately 48 hours from approximately 12UT July 12 to 12UT July 14. On July 14, an EUVE Target of Opportunity Observation was executed and a weak EUV source was detected in the ALEXIS error box that *could* be the fading or quiescent counterpart to the event. The EUV source was approximately 1 arcminute away from a 6.5 mag G6III star which may or may not be the EUVE source. The fitted centroid of the source in the EUVE data is located at: RA = 20 41 0.4 Dec = -42 23 25.3 (J2000) or RA = 310.25176 degrees Dec = -42.390355 degrees From SIMBAD the Info on the nearby bright star is: HD 196748 -- Star in double system Coordinates (2000.0) : 20 40 55.35 -42 23 49.2 Galactic coordinates : 358.76 -37.56 Pr. motion [error] (2000.0) : -0.004 [ 10] +0.010 [ 8] B magn:7.3 V magn:6.5 Pecul: Spectral type : G6III And it's double companion: CD-42 15029B -- Star in double system Coordinates (2000.0) : 20 40 53.8 -42 23 38 Galactic coordinates : 358.76 -37.56 B magn:11.6 V magn:9.7 Pecul: Spectral type : G5 We need someone with a view of this southern object(s) to take a high resolution Calcium H and K spectra of this star system to check for coronal activity. Thanks in advance for any assistance, Jeff Bloch -------------------------------------------------------------------------- Jeffrey Bloch Office: (505) 665-2568 Astrophysics and Radiation Measurements Group ALEXIS SOC:(505) 665-5975 Los Alamos National Laboratory FAX: (505) 665-4414 Group NIS-2, Mail Stop D436 e-mail: jbloch@lanl.gov Los Alamos, NM 87545 Digital Pager: (505)665-9800 #104-8074 --------------------------------------------------------------------------