Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 6103: 1994ad; GRO J0422+32

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 6102  SEARCH Read IAUC 6104

View IAUC 6103 in .dvi or .ps format.
IAUC number


                                                  Circular No. 6103
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)
Phone 617-495-7244/7440/7444     TWX 710-320-6842 ASTROGRAM CAM
MARSDEN@CFA.HARVARD.EDU or GREEN@CFA.HARVARD.EDU (science)


SUPERNOVA 1994ad IN ESO 152-G26
     R. H. McNaught, Anglo-Australian Observatory, reports his
discovery of an apparent supernova (mag about 18) in ESO 152-G26 on
an I plate taken on Nov. 10 by M. Hartley with the U.K. Schmidt
telescope.  Confirmation was obtained on Nov. 11 via a CCD image
taken by D. I. Steel and G. J. Garradd with the 1.0-m reflector at
Siding Spring Observatory.  Coordinates for the supernova were
measured by McNaught from the CCD image:  R.A. = 1h47m39s.57, Decl.
= -56o17'30".0 (equinox 1950.0, uncertainty in each coordinate
0".4); SN 1994ad is situated in a spiral arm and offset 0".6 west
and 33".9 north from the galaxy's center.  No image appears in this
position on the SERC J or the European Southern Observatory B and R
surveys.  A nearby star (about 0.5 mag fainter than the supernova)
has position end figures 42s.55, 18'14".8.


GRO J0422+32
     J. Orosz and C. Bailyn, Department of Astronomy, Yale
University, report:  "Optical observations of the black-hole
candidate GRO J0422+32 in quiescence confirm an orbital period of
5.06 hr and strongly suggest a velocity semi-amplitude for the
secondary star near 400 km/s.  This would imply a mass function for
the primary star of about 1.4 solar masses.  Photometry with the
Kitt Peak 2.1-m telescope (+ Tek CCD) on Oct. 27-28 confirms  the
quiescent magnitudes reported on IAUC 6072 and reveals a double-
humped ellipsoidal lightcurve with an amplitude of 0.1 mag in I and
a period of 0.2107 +/- 0.0012 day.  Spectra obtained with the Kitt
Peak 4-m reflector (+ RC spectrograph) on Nov. 5-7 show double-
peaked H-alpha and H-beta emission lines superposed on a continuum
displaying the broad TiO absorption bands typical of early-M-type
stars.  Profile fitting to the emission lines implies an outer-disk
velocity of 460 +/- 20 km/s; in previous x-ray novae, this value
has proved to be 10-20 percent greater than the velocity
semiamplitude of the secondary.  While velocity determinations could
not be obtained for individual spectra, sums of twenty-nine 1800-s
exposures (with velocity shifts determined from sinusoids with the
period given above, zero phase at Nov. 5.0025 UT, and
semiamplitudes between 370 and 430 km/s) provided strong cross-
correlations with a template star of spectral type M0 V."


1994 November 11               (6103)            Daniel W. E. Green

Read IAUC 6102  SEARCH Read IAUC 6104

View IAUC 6103 in .dvi or .ps format.


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


Valid HTML 4.01!