Circular No. 3790 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 617-864-5758 NOVA SERPENTIS 1983 T. Iijima, S. Ortolani and L. Rosino, Asiago Astrophysical Observatory, telex: "Spectra obtained with the 1.22-m and 1.82-m telescopes at Asiago during Mar. 3-19 show broad emission features of H, He I, He II 468.6 nm, N III 464.0 nm, and nebular forbidden lines of [O III] at 500.6 and 495.9 nm. The expansion velocity from the total halfwidth of the H emission bands is 4050 km/s. The H and He emission bands are formed by two broad, symmetric features with a peak separation of ~ 5400 km/s and a central narrower emission that also appears in the echelle spectrograms (dispersion 10.2 A/mm) to be double peaked (with the components separated by 530 km/s). The nova has already entered the nebular stage, and the excitation is increasing. In the last spectra of Mar. 19 He II 468.6 nm is stronger than H-beta." NO OCCULTATIONS BY URANUS II AND PLUTO P. Maley, Houston, TX, reports that he detected no occultation on Mar. 25 by Umbriel (cf. IAUC 3784) while observing at Oberon (!), N.S.W., during a 20-min interval beginning at 16h18m UT. He also reports negative observations by P. Anderson (near Brisbane) and by R. Price (100 km west of Canberra). Maley also informs us that no occultation by Pluto (cf. IAUC 3780) was observed from Houston during Apr. 4d07h23m-4d07h51m UT. TIME ADJUSTMENT ON 1983 JUNE 30 The Bureau International de l'Heure, Paris, informs us that a positive leap second will be introduced such that the sequence of UTC second markers will be: 1983 June 30d23h59m59s, 30d23h59m60s, July 1d00h00m00s. From 1982 July 1 to 1983 June 30 the difference UTC-TAI = -21s: beginning 1983 July 1 UTC-TAI = -22s. CORRIGENDUM IAUC 3784, Supernova in Anonymous Galaxy, line 3. For on read an. 1983 April 7 (3790) Brian G. Marsden
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