Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 4388: N Her 1987; 1987A; AM Her

The following International Astronomical Union Circular may be linked-to from your own Web pages, but must not otherwise be redistributed (see these notes on the conditions under which circulars are made available on our WWW site).


Read IAUC 4387  SEARCH Read IAUC 4389
IAUC number


                                                  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

Read IAUC 4387  SEARCH Read IAUC 4389


Our Web policy. Index to the CBAT/MPC/ICQ pages.


Valid HTML 4.01!