New eclipsing binaries

[Patrick Wils <patrickwils@yahoo.com>]

From the new list of suspected variables given by Tom, the data
revealed that the following stars are definitely new short period
variables (thanks to John Greaves I needed to check only a handful):

ID               V-Ic Type
J155818.6+481448 0.60  EA P=1.35d?
J162410.4+455528 0.95  EW
J163135.7+484336 0.48  EW:
J170121.8+420949 0.73  EW
J182247.0+443441 1.41  EW
J184510.7+284113 0.76  EW
J195916.3+363207 0.19  EW? Period may also be 2.2d
J202804.8+311709 0.32  EW
J203557.1+490042 0.99  EW
J204510.3+480512 0.51  EW
J204616.7+423522 0.75  EW
J211523.9+443745 1.03  EW

There is still more than one possible period for most of these stars.
Others may be short period variables as well, but with not enough data
points for the moment to be certain.
There are also a number of hitherto unknown obviously long period
variable stars in Tom's list, but these I have not looked into further.

Patrick


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