The Ritter Observatory classical Be star observational  program

        Summer 2002 (version 6)
Aim

Long-term monitoring of the spectral line behavior in order to study physics of circumstellar matter around Be stars in more detail, reveal the nature and mechanisms of the line variations. This program is being supported by optical photometry by collaborators in Kazakhstan  (since September 2001).
 

Observations obtained since June 25, 2002
 48 Lib  Delta Sco Chi Oph Omicron Her 66 Oph 12 Vul 60 Cyg   66 Cyg Pi Aqr Gam Cas Omi Cas
 weekly  nightly   weekly   weekly   weekly  weekly  weekly  weekly  nightly  nightly  nightly
  2400 s   900 s   1800 s   1800 s   1800 s   3000 s  3000 s  2400 s  3000 s   900 s   1800 s
 06/30,  99 06/25,287+370  06/25, 183 06/28,133+113  06/25, 181  06/29, 120  07/06, 126  06/25, 231  07/01, 126  06/25, 256 06/30, 144
 07/04, 207 06/29, 371  06/30, 152  07/02, 235  06/30, 109  07/05, 198  10/21, 161  06/30, 193  07/05, 188  06/30, 406 10/20, 184
 07/08, 221 06/30,173+225  07/06, 502  07/07, 185  07/06, 174  07/08, 209  10/31, 102  07/08, 362  07/08, 217  07/02, 491 10/29, 152
07/01, 451 10/23, 213 10/17, 147 07/03, 491 10/31, 230
07/02, 702 10/29, 141 07/07, 334
07/03, 420 10/20, 631
07/04, 480 10/21, 435
07/05, 641 10/29, 368
07/06,214+663 10/31, 333
07/07,393
07/08, 544
09/22, 199


Last updated: 2002 October 31