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[vsnet-newvar 2172] New probable EW type eclipsing binaries from TASS survey data



The following stars were found to be variable from TASS data
(http://vsnet.tass-survey.org) by Tom Droege (acknowledgements to John
Greaves for making the selection):

RA  2000  Dec    Vmax ampl V-Ic Type  Period    Epoch    Name
002827.9 +785742 10.1 0.5  0.65 EW    0.27383   52868.88 GSC 4500-730
154710.5 +530209  9.7 0.4  0.86 EW    0.28071   52824.61 GSC 3870-1172
162744.1 +564559 11.5 0.6  0.76 EW    0.28268   52808.69 GSC 3881-579
163216.6 +775411 11.7 0.7  0.65 EW    0.32429   52739.88 GSC 4571-663
171112.1 +683323 11.9 0.7  0.79 EW    0.22813   52817.68 GSC 4421-1217
172406.2 +735437 11.8 0.7  0.93 EW    0.46301   52823.70 GSC 4427-540
192104.5 +561941 10.6 0.4  0.66 EW    0.67210   52852.67 GSC 3929-1500
195021.3 +701714 11.0 0.5  0.85 EW    0.32410   52859.67 GSC 4449-995
210148.8 +504709 10.7 0.5  2.19 EW    0.33822   52876.68 GSC 3600-110
222122.2 +651600 11.2 0.6  0.83 EW    0.23695   52874.74 GSC 4272-249

Periods will probably need to be refined when more data becomes
available.

More information on these variables may be found at the following URLs
respectively:
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ002827.9%2b785742
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ154710.5%2b530209
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ162744.1%2b564559
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ163216.6%2b775411
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ171112.1%2b683323
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ172406.2%2b735437
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ192104.5%2b561941
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ195021.3%2b701714
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ210148.8%2b504709
http://wiki.tass-survey.org/tass/view.do?nodeId=Tass&contentId=TassJ222122.2%2b651600

Patrick


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