[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-alert 4502] (fwd) XTE J1118+480
- Date: Fri, 31 Mar 2000 01:40:06 +0900 (JST)
- To: vsnet-alert
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 4502] (fwd) XTE J1118+480
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
(fwd) XTE J1118+480
Date: Thu, 30 Mar 2000 11:21:41 -0500 (EST)
From: Ron Remillard <rr@space.mit.edu>
The RXTE All-Sky Monitor has detected X-ray emission from a new
source, XTE J1118+480. The ASM position (equinox 2000.0, with a 90%
confidence radius of 6') is centered at R.A. = 11h 18m 17s,
Decl. = +48o 03'.0 The average X-ray intensity (2-12 keV) is
39(8) mCrab on March 29. Retrospective ASM analysis indicates that the
X-ray flux has been slowly rising since March 5. Another modest outburst
had previously occurred during Jan 2-29 2000, peaking at 37(3) mCrab on
Jan 6. The SIMBAD database lists only an unremarkable guide star (V~11)
near the X-ray position. The source was confirmed in an 800 s
RXTE pointed observation beginning on 23:14 UT March 29. Rapid flares
(e.g. 10 s) were seen, reaching a factor of 5 above the baseline flux
near 25 mCrab and suggesting a Galactic X-ray source. No pulsations
were detected. The X-ray spectrum does not vary appreciably during
intense flares. Preliminary spectral analysis indicates a power-law
visible to 30 keV. The photon index is roughly 1.8, which is similar
to Cyg X-1 in its hard state. The high galactic latitude (62o)
and X-ray properties present a puzzling combination,
and observations at other wavelengths are urgently needed.
_____
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp