[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsolj-alert 422] XTE J1859+226
- Date: Wed, 13 Oct 1999 13:00:24 +0900 (JST)
- To: vsolj-alert@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsolj-alert 422] XTE J1859+226
- Sender: owner-vsolj-alert@ooruri.kusastro.kyoto-u.ac.jp
XTE J1859+226
X線新星ですが、可視光で15等の天体と同定されたようです。電波情報を送り
ます。詳細は後程?
From rhjellmi@zia.aoc.NRAO.EDU Wed Oct 13 05:05 JST 1999
Date: Tue, 12 Oct 1999 14:03:04 -0600
To: dasmith@space.mit.edu, michiel@astro.uva.nl, rpf@astro.uva.nl,
rudy@space.mit.edu, gehrels@lheavx.gsfc.nasa.gov,
giommi@napa.sdc.asi.it, jem@head-cfa.harvard.edu, lewin@space.mit.edu,
rr@space.mit.edu, shrader@grossc.gsfc.nasa.gov,
stroh@pcasun1.gsfc.nasa.gov, swank@pcasun1.gsfc.nasa.gov,
bmg@space.mit.edu, tkato@kusastro.kyoto-u.ac.jp,
HARMON@SSLMOR.msfc.nasa.gov, chaswell@star.cpes.susx.ac.uk,
ehm@space.mit.edu, Michael.McCollough@msfc.nasa.gov,
p.charles1@physics.oxford.ac.uk, eiken@astrosun.tn.cornell.edu,
srk@astro.caltech.edu, luisfr@astrosmo.unam.mx,
tavani@astro.columbia.edu, ewaltman@rsd.nrl.navy.mil,
fghigo@cv3.cv.nrao.edu, rmw@as.arizona.edu, mrupen@zia.aoc.NRAO.EDU,
amiodusz@zia.aoc.NRAO.EDU, mirabel@discovery.saclay.cea.fr,
S.Chaty@open.ac.uk, greiner@aip.de, mnowak@rocinante.colorado.edu,
wheel@alla.as.utexas.edu, garcia@head-cfa.harvard.edu,
satr@cats.sao.ru, vdhawan@zia.aoc.NRAO.EDU
From: "Robert M. (Bob) Hjellming" <rhjellmi@aoc.nrao.edu>
Subject: XTE J1859+226
Cc: rhjellmi@zia.aoc.NRAO.EDU
Mime-Version: 1.0
Content-Type: text/plain; charset="us-ascii"
Content-Length: 1374
Status: O
Collegues,
While we still need to make confirming observations with the VLA, this
is to notify you that XTE J1859+226 almost certainly has a radio counterpart.
I passed on the early warning of the PCA position circular in time for Guy
Pooley
to make an observation with the Ryle Telescope on Monday. He found a
new 14 mJy radio source at 15 GHz at a position of
J2000 18 58 31 +22 39 10
with at least 30" uncertainty in declination because it was a brief
observation
of a very southerly source observed with an E-W array. He hesitated making
a public announcement because of the adverse conditions of observation.
However,
the optical transient reported in IAUC 7276 is on this position, so we
think there is little doubt there was/is a radio counterpart to XTE J1859+226.
Guy and I had planned to wait until we have confirming results from the
VLA observations that will take place tonight (Oct. 12), but this seems
important enough to give you a heads-up that there is almost certainly
a radio counterpart. Guy told me I could pass his results on to anyone,
so I am doing so.
Barring a disaster at the VLA such as a power outage or online computer
failure, we should know what we have this evening and I will send out a report
- and we will do whatever is appropriate for IAUCs.
Bob Hjellming (on behalf of the XTE J1859+226 radio + ??? collaboration)
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp