Circular No. 3910 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 SUPERNOVA IN NGC 4419 L. Rosino, Asiago Astrophysical Observatory, telexes that spectra obtained on Jan. 9, 10 and 11 by Rafanelli and Iijima with the 1.82-m and 1.22-m telescopes match well with those of supernovae of type I, except that the typical absorption feature at 615 nm is blueshifted to 600 nm. The other emission and absorption features are all displaced toward the blue by ~ 8000 km/s relative to normal type-I supernovae. The following magnitudes were estimated from Asiago Schmidt plates on Jan. 10: V = 12.8, B-V = +0.3. PERIODIC COMET CROMMELIN (1983n) Several observers have noted that this test comet for the International Halley Watch continues to be a very difficult object. Only the following recent positions have been reported: 1984 UT R.A. (1950.0) Decl. m2 Observer Jan. 1.98703 21 36 41.57 + 6 10 34.6 18.5 McCrosky 3.08750 21 39 51.47 + 6 07 59.1 Everhart R. E. McCrosky (Oak Ridge Observatory). 1.5-m reflector. E. Everhart (Chamberlin Obs., field station). 0.4-m reflector. 1984 AB A minor planet recently discovered by E. Helin at Palomar seems to have an orbit (a = 1.53 AU, e = 0.086, i = 12 deg: see MPC 8467) resembling that of Mars. The observed arc is only 4 days, and the orbit could be rather larger (with a up to 1.9 AU), but the inclination would then be too high for a normal Hungaria object. This ephemeris is from MPC 8468: 1984 ET R.A. (1950.0) Decl. p r Mag. Jan. 1 6 11.73 +24 35.9 0.554 1.535 16.2 11 5 54.57 +27 35.0 21 5 41.28 +30 08.1 0.592 1.511 16.8 31 5 34.15 +32 11.0 Feb. 10 5 34.01 +33 47.5 0.691 1.487 17.3 20 5 40.52 +35 02.2 Mar. 1 5 52.75 +35 57.6 0.816 1.465 17.8 11 6 09.80 +36 33.7 21 6 30.71 +36 49.4 0.946 1.444 18.2 1984 January 16 (3910) Brian G. Marsden
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