2000ApJ...531..407C


Query : 2000ApJ...531..407C

2000ApJ...531..407C - Astrophys. J., 531, 407-410 (2000/March-1)

Observations of a possible new Soft Gamma Repeater, SGR 1801-23.

CLINE T., FREDERIKS D.D., GOLENETSKII S., HURLEY K., KOUVELIOTOU C., MAZETS E. and VAN PARADIJS J.

Abstract (from CDS):

We report on two 1997 June observations of a soft bursting source whose time histories and energy spectra are consistent with those of the soft gamma repeaters. The source can be localized only to an ~3°.8 long error box in the direction of the Galactic center, whose area is ~80 arcmin2. The location of the source, while not consistent with that of any of the four known soft repeaters, is consistent with those of several known and possible supernova remnants.

Abstract Copyright:

Journal keyword(s): Gamma Rays: Bursts - Stars: Neutron - ISM: Supernova Remnants - X-Rays: Stars

Nomenclature: NAME SGR 1801-23

Simbad objects: 17

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Number of rows : 17
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 GAL 005.4-00.29 SR? 17 59 -24.4           ~ 1 0
2 GAL 007.4+00.7 SR? 18 00 -22.2           ~ 1 0
3 SNR G006.4-00.1 SNR 18 00 31.2011719 -23 25 48.001099           ~ 737 1
4 RAFGL 2046 HII 18 00 32.1 -24 04 03           ~ 361 0
5 NAME Sgr 1801-23 gam 18 00 58.9 -22 56 48           ~ 37 0
6 SNR G007.2+00.2 SNR 18 01.1 -22 38           ~ 16 0
7 PSR B1758-23 Psr 18 01 19.8149 -23 04 44.630           ~ 143 0
8 GAL 007.4+00.05 SR? 18 02 -22.5           ~ 1 0
9 NAME Duck Redux Rad 18 02 10.000 -24 54 00.00           ~ 179 3
10 1WGA J1802.3-2151 X 18 02 19.3 -21 51 57           ~ 1 0
11 GRS G008.10 +00.20 Rad 18 02 58.8 -21 49 54           ~ 7 0
12 GAL 007.0-00.3 SR? 18 03 -23.1           ~ 1 0
13 PSR B1800-21 Psr 18 03 51.45 -21 37 08.1           ~ 260 1
14 [GS70] 006.0-01.2 Rad 18 04 -24.4           ~ 1 0
15 W 30 BL? 18 05 31.2011719 -21 25 48.001099           ~ 174 1
16 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1240 2
17 GBS 1900+14 gB 19 07 13 +09 19.6           ~ 857 0

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