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THE ASTRONOMER Electronic Circular No 1343      1998 Oct 04 13.20UT
Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise,  Basingstoke,
Hants, RG22 4PP,England.Telephone/FAX(01256)471074Int:+441256471074
INTERNET: GUY@TAHQ.DEMON.CO.UK             GMH at AST.STAR.RL.AC.UK
WORLD WIDE WEB                    http://www.demon.co.uk/astronomer
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V751 CYGNI
During his recent presentation at the TA AGM in Birmingham, Gary
Poyner appealed for more observations of the nova-like variable
V751 Cygni which has a catalogued range of 13.8-16.3p and which
is currently near the brighter end of its amplitude. A paper TA
chart version of the field has been existence for many years, but
we have now upgraded the sequence against new V values by Henden
and Honeycutt and also produced an e-chart shown below:
\\\\\\V751 Cyg  c        NSV 13378 8.3-9.0p also
S,400,5,S
-C,20.8703, 44.3236,2000
O,200,200,13.8,16.3p
-L,L,V751
-T,Nova-Like?;Seq V by Henden
-S,TA981004
P,20h 52.2m  +44 19'  (2000)
M,4,332,154
-L,L,Fl 57
M,8,193,120
-L,L,NSV 13378
R,12.28,181,175,3
R,13.50,185,226,5,R
R,13.55,204,204,7,R
R,14.2,176,230,W
R,15.42,214,191,9,R
R,16.10,207,196,8,R
M,9,381,232,97,333,251,123,244,293
M,10,166,278,206,321,66,391,188,388,298,345
M,11,272,14,378,32,232,77,375,323,20,363,295,320,123,262
M,11,331,235,26,113,337,392
M,12,299,252,76,133,349,190,96,134,28,286,305,388
M,12,348,99,64,168,292,255,41,25,105,380,104,304,309,293
M,12,206,284,107,205,247,98,24,78,151,369,124,372,43,369
M,12,282,48,384,138
M,13,88,14,318,316,149,390,299,125,94,125,375,253
M,13,282,121,321,79,377,159,18,222,106,302,110,144,196,156
M,13,297,105,77,322,63,159,312,75,319,11,100,174,394,342
M,13,35,178,71,208,215,263,71,181,349,38,280,204,76,136
M,13,195,381,232,40,172,325,192,279,184,150,106,338,94,43
M,13,130,151
M,14,35,179,36,199,358,368,32,346,362,365,76,135,27,267
M,14,178,155,347,361,89,144,247,131,121,143,221,15,69,345
M,14,52,293,307,198,391,50,63,130,233,349,241,226,224,31
M,14,229,228,148,130,276,158
E,109
////// Basic chart automatically generated by CHART ver 1.6

Please make observations of this variable whenever possible.

Guy M Hurst