.dvi
or
.ps
format.
Circular No. 6853 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) BMARSDEN@CFA.HARVARD.EDU or DGREEN@CFA.HARVARD.EDU (science) URL http://cfa-www.harvard.edu/iau/cbat.html Phone 617-495-7244/7440/7444 (for emergency use only) GRB 980329 F. Frontera, Istituto Tecnologie e Studio Radiazioni Extraterrestri, Bologna; E. Costa, L. Piro, and P. Soffitta, Istituto Astrofisica Spaziale, CNR, Rome; J. in 't Zand, Space Research Organization of the Netherlands (SRON), Utrecht; L. Di Ciolo and A. Tesseri, BeppoSAX Science Operation Center (SOC), Rome; and M. Smith, SOC and SRON report: "The BeppoSAX Gamma Ray Burst Monitor was triggered by a gamma-ray burst on Mar. 29.1559 UT, corresponding to BATSE trigger 6665. A preliminary analysis shows a duration of 15 s and a peak intensity of 6000 counts/s (40-700 keV). This is the brightest burst detected so far by the BeppoSAX GRBM simultaneously with the Wide Field Cameras (WFC). The peak intensity measured in the WFC is about 6 Crab (2-26 keV). The source position is R.A. = 7h02m41s, Decl. = +38o50'.7 (equinox 2000.0; error radius 3'). A BeppoSAX follow-up observation is in progress." AX J0051-73.3 AND AX J0058-72.0 J. Yokogawa and K. Koyama, Kyoto University, report: "ASCA detected two new x-ray pulsars in the Small Magellanic Cloud, designated AX J0051-73.3 and AX J0058-72.0. AX J0051-73.3 was detected on 1997 Nov. 13 at R.A. = 0h50m47s, Decl. = -73o15'51" (equinox 2000.0; +/- 1' at 90-percent confidence), with a pulse period of 323.2 +/- 0.4 s and a quasi-sinusoidal pulse shape. Its spectrum was well fitted with a power law having a photon index of 0.6 +/- 0.2; the x-ray flux in the band 0.7-10.0 keV was 3.6 x 10E-12 erg sE-1 cmE-2. AX J0058-72.0 was detected on 1997 Nov. 14 at R.A. = 0h57m57s, Decl. = -72o02'46" (equinox 2000.0; +/- 1' at 90-percent confidence). Its pulse period was 280.4 +/- 0.3 s, with a single-peaked pulse shape; its spectrum was well fitted with a power law having a photon index of 1.0 +/- 0.3, and its x-ray flux in the band 0.7-10.0 keV was 2.4 x 10E-12 erg sE-1 cmE-2." SUPERNOVAE 1997dq AND 1998W S. Moretti and S. Tomaselli, Forli, Italy, report the following unfiltered CCD magnitude estimates using GSC reference stars: SN 1997dq in NGC 3810 (cf. IAUC 6770), Mar. 26.92 UT, 17.6; SN 1998W in NGC 3075 (cf. IAUC 6843), Mar. 26.91, 17.1. (C) Copyright 1998 CBAT 1998 March 30 (6853) Daniel W. E. Green
.dvi
or
.ps
format.
Our Web policy. Index to the CBAT/MPC/ICQ pages.