Telescopic LPVs for New Visual Observers
By Mike Simonsen,
Maybe you were drawn in by the Citizen Sky project and now you’re getting hooked on variable stars. Hey, it happens; you are not alone.
R Cas- This Mira gets as bright as 4.7, and can fade to 13.5.
T Cas- When at or near maximum, this is one of the reddest stars you’ll ever see in the eyepiece. This Mira varies from 6.9-13.0V and has a very interesting light curve with multiple humps, perhaps indicating multiple periods. Have fun following this one! T Cas has humps like a camel in its light curve. What's up with that?
S Per- Sitting in a beautiful star field with plenty of 8th and 9th magnitude stars to point the way, this interesting semi-regular variable, varying from 7.9-12V, is somewhat unpredictable, so you never know what it will be doing next time you observe it.
W Tau- Located in the Hyades, just west of Aldebaran is a bright double star consisting of theta 1 and theta 2 Tau. In the same medium power field of view is W Tau, a semi-regular variable that ranges from 8.2-13.0V. The period is listed as approximately 165 days, but this star is unpredictable, and the light curve for the last 1200 days is chaotic. This, plus the fact it is easy to find and observe, makes W Tauri a fine catch on a cold winter night. W Tau is close to a beautiful double star in the Hyades cluster. You gotta be able to find this one!
There you go; a half dozen stars to add to your variable star program. If you’re looking for more you can check out the Stars Easy to Observe list on the AAVSO website at http://www.aavso.org/easy-stars.