Thom Gandet wrote: >>Delta Sco, considering its spectral type, its past spectroscopic behavior and its recent photometric behavior, may be a Herbig Be star rather than a classical Be star. The prior lack of convincing evidence for a spectroscopic period ought to be re-examined, as the recent photometry by Sebastian and others (IBVS 5026) does show evidence for a period near 80-days. However, it is difficult to measure radial velocities of Be stars that are meaningful in terms of Keplerian motion because of effects by gas streams, decretion/ accretion disk activity, etc. Dear friends: Tonight I observed delta Scorpii and Thom's words seem to ring true. The star is rising again and the activity is always in agreement with a 72 - 77 day period, slightly shorter than proposed by Thom. I supposed the star was going to fade at last, but the fading stopped near JD 2452015 that is exactly 3 cycles of 73 days later than the first well-observed 2.15 minimum. The star has brightened by 0.05 magnitudes and it is very interesting to take a look at the following table with maxima and minima. (JD's are approximated [little gaps in the data] but they can't be off by more than 5 days) FIRST CYCLE: Maximum 1.91 - JD 2451752 Minimum 2.15 - JD 2451793 SECOND CYCLE: Maximum 1.85 - JD 2451824 Minimum ?? THIRD CYCLE: The star was not visible !! FOURTH CYCLE: Maximum 1.80 - JD 2451978 Minimum 1.85 - JD 2452015 Tonight's observation is 1.81 again, and this means that the star will probably be VERY bright in a 20-25 days time. (maybe 1.7?). I really don't know if there is a companion in a 75 day orbit inducing light changes but the changes are there. Maybe with another cycle going on as predicted, more can be said... In 25 days we'll have another clue. Best regards, Sebastian Otero, LIADA. --- Outgoing mail is certified Virus Free. Checked by AVG anti-virus system (http://vsnet.grisoft.com). Version: 6.0.249 / Virus Database: 122 - Release Date: 13/04/01