2011ATel.3663....1P


Query : 2011ATel.3663....1P

2011ATel.3663....1P - The Astronomer's Telegram, 3663, 1 (2011/September-0)

Swift Detection of an Intermediate Duration Burst from SAX J1712.6-3739.

PALMER D.

Abstract (from CDS):

On September 26, 2011, 20:11:28 UT, BAT detected high flux from a location consistent SAX J1712.6-3739, an LMXB. Swift slewed immediately to the source. The BAT on-board calculated location is

(RA, Dec) = (258.161, -37.649) = (17h 12m 39s, -37d 38' 56") (J2000)

with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty).

Based on downlinked BAT data from T-120s to T+300s, the emission started

at T-75s, rising smoothly to a peak at T+100s, and declining to near zero at T+200s. The counts are almost all in the 15-25 keV band. Over

the time interval T-74s to T+188s the data are well-fit by OTTB (T∼4.7 keV) or Blackbody (T∼2.7 keV) models with fluence above 15 keV of ∼1.7x10^-6 erg/cm^2

The XRT began observing the field at 20:13:25.9 UT, 117.4 seconds after the BAT trigger. XRT found a bright X-ray source located at

(RA, Dec) = (258.1528, -37.6469) = (17h 12m 36.67s, Dec(J2000) = -37d 38' 48.8") (J2000)

with an uncertainty of 5.9 arcseconds (radius, 90% containment). This position is 15.6 arcseconds from the catalogued location of a known X-ray source: 1RXS J171237.1-373834 in the ROSAT RASSBSC catalogue (identified by SIMBAD with SAX J1712.6-3739 and positionally consistent

within the joint ROSAT-XRT uncertainty).

The XRT light curve shows near-constant emission until ∼T+220s, followed

by high-amplitude variation on multiple timescales for at least 7 minutes. Over T+120s to T+800s, the XRT spectrum is well fit by an absorbed black-body, kT=2.18 ± 0.07 keV and N_H = 1.69 ± 0.14 x 10^22 cm^-2. The average absorption-corrected flux is ∼2x10^-8 erg/s/cm^2.

This timescale indicates that event is an intermediate duration burst (typical timescale ∼30 minutes), not a superburst (typical timescale ∼10

hours), and not an ordinary Type I burst (typical timescale ∼10 seconds). (See Cumming et al. 2006, ApJ 646, 429.)

The history of this source includes an ordinary Type I burst seen by BAT in July 2010 (ATel #2717; Strohmeyer & Baumgartner, 2010) and an intermediate duration burst in 1999 found in RXTE/ASM archival data (ATEL #2141; Kuulkers, 2009).


Abstract Copyright: ∼

Journal keyword(s): Gamma Ray - Neutron Star - Transient

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 [KRL2007b] 228 LXB 17 12 37.0 -37 38 42     12.25     ~ 81 0

Query : 2011ATel.3663....1P

Basic data :
[KRL2007b] 228 -- Low Mass X-ray Binary
Other object types:
otypes_help
X (2022MNRAS,PBC,...), LXB (2013ApJS), gam (INTEGRAL1,INTREF), N*? (2007ApJS), V* (2012A&A)
ICRS coord. (ep=J2000) :
17 12 37.0 -37 38 42 (X-ray) [ 5000 5000 90 ] D 2022A&A...661A..38P
FK4 coord. (ep=B1950 eq=1950) :
17 09 12.9 -37 35 09 [ 5000 5000 90 ]
Gal coord. (ep=J2000) :
348.9391 +00.9185 [ 5000 5000 90 ]
Fluxes (1) :
V 12.25 [0.07] C 2012A&A...548A..79A
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Identifiers (10) :
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INTEGRAL1 47 1RXS J171237.1-373834 SWIFT J1712.8-3737 [KRL2007b] 228
INTREF 758 SAX J1712.6-3739 SWIFT J1712.6-3736
PBC J1712.6-3737 SRGA J171237.0-373843 XMMSL1 J171236.3-373841

References (81 between 1850 and 2026) (Total 81)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Distance : 1   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : [KRL2007b] 228

Link by name to the catalogue in VizieR :

1RXS J171237.1-373834

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