[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]

[vsnet-alert 7823] (fwd) V4641 Sgr, also active in X-rays!



(fwd) V4641 Sgr, also active in X-rays!

Date: Wed, 6 Aug 2003 22:53:05 -0400 (EDT)
From: Charles Bailyn <bailyn@astro.yale.edu>
Subject: X-ray observations of V4641 Sgr

As you see below, there is exciting activity in the X-ray as well.
More X-ray observations are scheduled for the next few days, so
please encourage everyone to keep looking at this source!

- Charles Bailyn


------------------------------------------------------------------------------
The Astronomer's Telegram			      http://atel.caltech.edu/
==============================================================================
ATEL #171							     ATEL #171

Title:		X-ray and Optical Activity in V4641 Sgr (=SAX 1819.3-2525)
Author:		C. Bailyn, D. Maitra, M. Buxton, L. Jeanty (Yale), D. Gonzalez
		(CTIO)
Queries:	bailyn@astro.yale.edu
Posted:		6 Aug 2003;  22:55  UT
Subjects:	Infra-Red, Optical, X-ray, Black Holes, Transients

V4641 Sgr is now active in X-rays, and activity continues in optical/IR
bands.  A ~1 kilosecond  dwell with the RXTE/PCA taken August 5 2003 starting
at UT 01:18 shows flux varying from 20 to   35 mCrabs.  On August 6 between
UT 08:43 - 09:31 the source was in a highly active flaring state, with
flares of up to 100 mCrabs erupting on timescale of 10-30 seconds.  Observations
on August 6 from   UT 10:23 - 11:13 did not show large flares, but rather
a state similar to that observed in the   August 5 dwell.  Similar activity
was also seen in optical/IR observations by the SMARTS consortium, using
the 1.3m telescope at CTIO with the ANDICAM instrument. On August 6 the
source brightened in the  V band from magnitude 12.4 to 10.9 between UT
00:00 and UT 05:15.  The source became somewhat bluer during this rise:
over the same period the K band brightened by only 1.1 magnitudes.  Flares
and dips of several tenths of a magnitude were observed on timescales of
<3 minutes.    


Return to Home Page

Return to the Powerful Daisaku Nogami

vsnet-adm@kusastro.kyoto-u.ac.jp

Powered by ooruri technology