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THE ASTRONOMER Electronic Circular No 850       1994 June 9 19.36UT
Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise,  Basingstoke,
Hants, RG22 4PP,England. Telephone/FAX(0256)471074 Int:+44256471074
INTERNET: GMH at AST.STAR.RL.AC.UK  or    GMH at GXVG.AST.CAM.AC.UK
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SUPERNOVA 1994R IN IC 2627
Ralph Martin and Andrew Williams, running the Perth Astronomy
Research Group automated supernova search on the 0.61-m
Perth-Lowell reflector, report their discovery on June 3.59 UT of a
supernova (mag about 16) located 21".5 west and 1".2 north of the
centre of IC 2627 (R.A. = 11h07m26s, Decl. = -23o27'.3, equinox
1950.0).  The new object was not visible on May 2.  C. Pollas,
Observatoire de la Cote d'Azur, reports that a poor image obtained
on June 3.87 shows SN 1994R to be new compared with the POSS prints
and at the brightness and location described above. S. Benetti,
ESO, reports that inspection of a preliminarily reduced CCD
spectrum (range 370-700 nm, resolution 2 nm) obtained on June
4.15 with ESO 3.6-m telescope (+ EFOSC1), confirms that the object
is a supernova of type II.
IAUC 6003

PROBABLE SUPERNOVA IN NGC 4495 (=Q1994/051)
Further to our appeal for confirmation of a possible supernova in
NGC 4495, it appears this object, reported by Larry Mitchell,
Houston, Texas is indeed a supernova. His discovery on June 4
yielded a visual estimate of about 14.5 (0.60-m reflector x333).
Brian Skiff has confirmed the new object using the Lowell 1.1-m
Hall telescope at CCD. He finds that V=14 and the offset about
20 arcseconds in pa250. The galaxy is located at:
RA 12h31m23.1s DEC +29 08'13"[2000] according to Dressel and
Condon.
Alejandro Clocchiatti reports via the novanet that Derek Wills
of McDonald Observatory has a spectrum which confirms the
object as a supernova. No designation or announcement has as yet
been made by the Central Bureau.

Guy M Hurst







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Date: Fri, 10 Jun 94 08:26:14 -0400