[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-alert 1926] New X-ray transient (Levine)
- Date: Mon, 29 Jun 1998 15:46:24 +0900 (JST)
- To: vsnet-alert
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 1926] New X-ray transient (Levine)
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Date: Sun, 28 Jun 1998 13:52:54 -0400 (EDT)
From: "Alan M. Levine" <aml@scox1.mit.edu>
Message-ID: <vsnet-alert1926@hoge.baba.hajime.jp>
To: aml@scox1.mit.edu, rr@scox1.mit.edu, ehm@scox1.mit.edu, cui@scox1.mit.edu,
hale@scox1.mit.edu, deepto@scox1.mit.edu, jgj@scox1.mit.edu,
dasmith@scox1.mit.edu, shirey@scox1.mit.edu, chekov@scox1.mit.edu,
muno@scox1.mit.edu, lqw@scox1.mit.edu, rhjellmi@aoc.nrao.edu,
jgreiner@aip.de, guy@mrao.cam.ac.uk, rpf@astro.uva.nl,
shrader@grossc.gsfc.nasa.gov, chen@tgrs.gsfc.nasa.gov,
rmw@lowell.Lowell.Edu, garcia@head-cfa.harvard.edu,
nagase@astro.isas.ac.jp, ueda@astro.isas.ac.jp,
dotani@astro.isas.ac.jp, saxsci@alpha1.ias.rm.cnr.it,
giommi@sax.sdc.asi.it, stella@coma.mporzio.astro.it,
filippo@tesre.bo.cnr.it, jeanz@purple.sron.ruu.nl, Michel.Boer@cesr.fr,
broberts@cea.berkeley.edu, costa@ias.rm.cnr.it, feroci@ias.rm.cnr.it,
swank@pcasun1.gsfc.nasa.gov, vsnet-alert@kusastro.kyoto-u.ac.jp,
xtesof@athena.gsfc.nasa.gov
Precedence: list
X-Distribute: distribute [version 2.1 (Alpha) patchlevel=24]
X-Sequence: vsnet-alert 0
Subject: [vsnet-alert 0] New transient X-ray source
Errors-To: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear observers & colleagues:
Here is advance notice of a new transient that we have found with
RXTE. It may be a good opportunity for followup observations. Good
luck!
I intend to submit copy to the IAU circulars later today or early
tomorrow AM at the latest.
-- Al Levine
Draft IAU Circular submission:
XTE J2123-058
A. Levine (MIT), J. Swank and E. Smith (GSFC) report on behalf of
the RXTE ASM and PCA teams at MIT and NASA GSFC:
A transient X-ray source has been detected with the RXTE/ASM at a
position: R.A. = 320.78 d, Dec. = -5.82 d (J2000) corresponding to l =
46.4 d, b = -36.2 d. The position uncertainty is about 10 arcmin
along an axis with position angle 20 deg. (i.e., NE-SW) and about 5
arcmin in the perpendicular direction (90% confidence) The flux was
measured to be ~100 mCrab (2 - 12 keV) in each of 5 measurements on
1998 June 27 - 28.
The strength of the source has been confirmed with PCA observations
June 27.95 in which the count rate varied from 600 to 1000 cts/s.
Additional PCA observations, including a determination of the source
location, will be undertaken.
The appearance of a new transient X-ray source at high galactic
latitude is unusual; we urge observers to carry out additional
observations at all wavelengths.
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp