Circular No. 4388 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. TWX 710-320-6842 ASTROGRAM CAM Telephone 617-495-7244/7440/7444 NOVA HERCULIS 1987 Y. Andrillat, Laboratoire d'Astronomie, Universite des Sciences et Techniques du Languedoc, Montpellier; and L. Houziaux, Institut d'Astrophysique, Universite de Liege, telex: "On a IIaO plate (resolution 8 nm/mm) obtained on May 6 and 7 at Observatoire de Haute Provence, Nova Her 1987 already reveals characteristic features of the nebular stage 96 days after maximum. [O III] lines are the most conspicuous features along with N III (464 nm); they exhibit a peaked profile with a FWHM of 2100 km/s. Balmer lines H-beta to H12 show a saddle-shaped emission typical of polar blobs geometry viewed from an angle of 30 deg-40 deg; their widths indicate an ejection velocity of about 2000 km/s. Emission at the Balmer limit is clearly noticeable. Other weaker identified features include He II (468.6 nm), N III (451 nm), C II (426.7 nm), [Ne III] (368.8 nm), and [Ne V] (342.6 and 334.6 nm)." Further visual magnitude estimates (cf. IAUC 4371): Apr. 10.09 UT, 10.8 (A. Pereira, Linda-A-Velha, Portugal); 18.10, 10.8 (Pereira); 22.06, 10.8 (P. Schmeer, Bischmisheim, West Germany); 26.09, 10.9 (Pereira); May 1.10, 11.0 (M. Verdenet, Bourbon-Lancy, France); 8.15, 11.2 (Pereira); 12.15, 11.3 (Pereira). SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD P. Whitelock, South African Astronomical Observatory, reports that SAAO photometry up to May 8 indicates that the V magnitude has reached a maximum or plateau; the infrared and bolometric flux continues to brighten, although the rate of brightening has decreased. Provisional photoelectric photometry by A. Beresford, Adelaide, S. Australia (0.20-m Schmidt-Cassegrain reflector): May 9.41 UT, V = 2.89, B-V = +1.58. Visual magnitude estimates: May 9.41 UT, 2.9 (Beresford); 11.41, 2.8 (R. H. McNaught, Coonabarabran, N.S.W.). AM HERCULIS Visual magnitude estimates: 1986 Sept. 21.82 UT, 14.2 (R. Monella, Covo, Italy); Oct. 5.8, 13.5 (A. Mizser, Budapest, Hungary); Nov. 3.8, 14.2 (Mizser); Dec. 15.75, 13.5 (Monella); 1987 Feb. 21.1, 13.0 (Mizser); Apr. 25.87, 13.4 (M. Verdenet, Bourbon- Lancy, France); 30.88, 13.1 (Verdenet). 1987 May 12 (4388) Daniel W. E. Green
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