[vsnet-alert 20805] OV Boo: time-resolved spectroscopy

[Keisuke Isogai]

OV Boo: time-resolved spectroscopy

     Saito and Ohshima (Nishi-harima Observatory) have reported the
time-resolved spectroscopies of OV Boo on Mar. 17 with the exporser times
of 600 sec.
     The spectra show double-peak H-alpha emissions, which was generated
in the disk. The profiles of the emissions have changed through the phase.
     The purpose of the time-resolved spectroscopy is the reconstruction of
the disk by Doppler tomography. So the population of OV Boo has not been
confirmed yet.