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[vsnet-alert 7417] (fwd) V4641 Sgr re-appears as a radio source!
- Date: Wed, 26 Jun 2002 22:11:58 +0900
- To: vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp, vsnet-campaign@ooruri.kusastro.kyoto-u.ac.jp
- From: Makoto Uemura <uemura@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-alert 7417] (fwd) V4641 Sgr re-appears as a radio source!
- Sender: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
------- Forwarded Message
Date: Wed, 26 Jun 2002 07:06:30 -0600
From: Michael Rupen <mrupen@aoc.nrao.edu>
To: vsnet-adm@kusastro.kyoto-u.ac.jp
Subject: V4641 Sgr re-appears as a radio source!
Dear colleagues,
we've just submitted an IAU circular, reporting renewed radio activity
in V4641 Sgr in mid- to late-June (latest detection was on 24jun02). This
contrasts with several years of roughly-monthly monitoring at the VLA, which
until the May outburst detected nothing to rms levels of order 50-150 microJy/beam.
The current detections, showing variability up to a factor 100 in flux density on
timescales less than a day, therefore represent a new state for this object.
Continued optical, X-ray, and radio monitoring is of great interest. I would
also be very interested to hear of any constraints on short timescale variability
in June...
Cheers,
Michael Rupen
NRAO/Socorro
mrupen@nrao.edu
------- End of Forwarded Message
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp