THE ASTRONOMER Electronic Circular No 516       1991 Apr 30 18.36UT
Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise,  Basingstoke,
Hants, RG22 4PP, England. Telephone:  (0256)471074 Int:+44256471074
Telex: 9312111261 Answerback: TA G                     JANET BOXES:
GMH at UK.AC.CAM.ASTRONOMY.STARLINK or GUYH at UK.AC.SUSSEX.CLUSTER
TELECOM GOLD: 10074:MIK2885                       PRESTEL 256471074
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EX HYDRAE
Brian Marsden relays a report from F.M.Bateson, Royal Astronomical
Society of New Zealand that this dwarf nova (RA 12h49m43s
DEC -28 58.7, 1950) is having a rare outburst. A.F.A.L.Jones of
Nelson has: Apr. 28.33UT, 10.1; 29.34, 10.6; 28.35, 10.4. The
last outburst was reported in 1987 (IAUC 4383, 4385, 4387).

SUPERNOVA 1991T IN NGC 4527
Further estimates reported (cf E513):
 910420.910, 11.7 pv  M Mobberley
 910420.927, 11.9 v   S Korth
 910420.930, 11.9 v   K Andersson
 910420.930, 12.0 v   B Granslo
 910420.948, 11.8 v   D Moore
 910420.990, 11.8 v   A Pereira
 910421.020, 12.0 v   G Poyner
 910421.035, 12.0 v   P Schmeer
 910421.520, 11.8 V   A Gilmore
 910421.887, 11.9 v   P Schmeer
 910421.896, 11.9 v   S Korth
 910421.900, 11.7 v   J Toone
 910421.930, 11.7 v   G Poyner
 910421.940, 12.2 v   M Villi
 910422.006, 11.9 v   P Schmeer
 910422.037, 11.9 v   H Mikuz
 910422.081, 11.3 v   D Moore
 910422.120, 11.6 v   G Lubcke
 910422.130, 11.6 v   P Steffey
 910422.868, 11.8 v   G Hurst
 910422.875, 11.7 v   G Hurst
 910422.895, 11.5 v   J Toone
 910422.900, 11.3 v   G Poyner
 910422.903, 11.5 v   W Worraker
 910422.940, 11.4 v   B Granslo
 910423.049, 11.8 pv  H Mikuz/A Dolzan
 910423.100, 11.4 v   P Steffey
 910423.872, 11.7 v   P Schmeer
 910424.150, 11.3 v   G Lubcke
 910424.872, 11.5 v   P Schmeer
 9104r5.915, 12.1 v   S Korth
 910425.924, 12.2 V   H Mikuz
 910427.899, 11.4 v   J Toone

NOVA IN THE LARGE MAGELLANIC CLOUD 1991
A. C. Gilmore reports the following photometry obtained with the
0.6-m Cassegrain reflector at Mt. John University Observatory on
Apr. 21.39 UT:  V = 10.23 +/- 0.01, U-B = -0.8 +/- 0.2, B-V = 0.00
+/- 0.01, V-R = +0.11 +/- 0.01, V-I = +0.18 +/- 0.03.
W. Liller, Vina del Mar, Chile, notes that this nova is now the
brightest one seen in the LMC; its peak absolute magnitude is ex-
pected to equal approximately that of V1500 Cyg.  Visual magnitude
estimates (those by Liller are photovisual):  Apr. 19.001 UT, 12.5
(Liller); 19.98, 11.8 (Liller); 21.04, 10.4 (Liller); 21.99, 9.8
(Liller); 23.76, 8.8 (T. Cooper, Benoni, R.S.A.); 24.73, 9.2
(Cooper); 24.77, 9.0 (D. Overbeek, Edenvale, R.S.A.).
IAUC 5250

Guy M Hurst