2018ApJ...854..125T

Query : 2018ApJ...854..125T

2018ApJ...854..125T - Astrophys. J., 854, 125-125 (2018/February-3)

A radio frequency study of the accreting millisecond X-ray pulsar, IGR J16597-3704 in the globular cluster NGC 6256.

TETARENKO A.J., BAHRAMIAN A., WIJNANDS R., HEINKE C.O., MACCARONE T.J., MILLER-JONES J.C.A., STRADER J., CHOMIUK L., DEGENAAR N., SIVAKOFF G.R., ALTAMIRANO D., DELLER A.T., KENNEA J.A., LI K.L., PLOTKIN R.M., RUSSELL T.D. and SHAW A.W.

Abstract (from CDS):

We present Karl G. Jansky Very Large Array radio frequency observations of the new accreting millisecond X-ray pulsar (AMXP), IGR J16597-3704, located in the globular cluster NGC 6256. With these data, we detect a radio counterpart to IGR J16597-3704, and determine an improved source position. Pairing our radio observations with quasi-simultaneous Swift/XRT X-ray observations, we place IGR J16597-3704 on the radio-X-ray luminosity plane, where we find that IGR J16597-3704 is one of the more radio-quiet neutron star low-mass X-ray binaries known to date. We discuss the mechanisms that may govern radio luminosity (and in turn jet production and evolution) in AMXPs. Furthermore, we use our derived radio position to search for a counterpart in archival Hubble Space Telescope and Chandra X-ray Observatory data, and estimate an upper limit on the X-ray luminosity of IGR J16597-3704 during quiescence.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): globular clusters: individual: NGC 6256 - ISM: jets and outflows - radio continuum: stars - stars: individual: IGR J16597-3704 - stars: neutron - X-rays: binaries

Simbad objects: 28

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Number of rows : 28
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 4U 0513-40 LXB 05 14 06.59 -40 02 37.0           ~ 176 1
2 MAXI J0556-332 LXB 05 56 46.32 -33 10 28.2           ~ 94 0
3 V* V1055 Ori LXB 06 17 07.3565603963 +09 08 13.515857360   18.80 18.5     ~ 594 1
4 MAXI J0911-655 Psr 09 12 03.4 -64 51 59           ~ 50 0
5 4U 0919-54 LXB 09 20 26.4818170056 -55 12 24.512806404 20.40 21.30 21.0     ~ 175 0
6 V* BW Ant LXB 09 29 20.19 -31 23 03.2   18.50 18.63     ~ 194 0
7 PSR J1023+0038 Psr 10 23 47.6841824712 +00 38 41.005893516     17.31     GV 470 0
8 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
9 V* QU TrA LXB 15 47 53.6 -62 34 11           ~ 168 0
10 V* HZ Her LXB 16 57 49.8110126616 +35 20 32.486555472 11.90 14.89 13.63 13.88   B3/6ep 2172 0
11 NGC 6256 GlC 16 59 32.68 -37 07 17.1           ~ 182 0
12 IGR J16597-3704 gam 16 59 32.90230 -37 07 14.2780           ~ 30 0
13 [KRL2007b] 214 LXB 17 00 58.46 -46 11 08.6           ~ 296 0
14 ICRF J171738.6-394852 Rad 17 17 38.59990175 -39 48 52.6653049           ~ 16 0
15 NAME Slow Burster LXB 17 31 58.0 -33 49 58     15.50     ~ 865 1
16 V* V2116 Oph Sy* 17 32 02.1532435416 -24 44 44.129169096   20.78 18.4     M6IIIe 719 1
17 NAME Rapid Burster LXB 17 33 24.0 -33 23 19           ~ 429 2
18 NAME TER 5 X-1 LXB 17 48 05.225 -24 46 47.66           ~ 229 1
19 [PLV2002] CX1 LXB 17 48 52.163 -20 21 32.40           ~ 213 1
20 IGR J17511-3057 LXB 17 51 08.55 -30 57 41.7           ~ 114 1
21 [KRL2007b] 291 LXB 17 51 13.49 -30 37 23.4           ~ 262 0
22 SWIFT J175233.9-290952 X 17 52 33.97 -29 09 52.3           ~ 9 0
23 SAX J1808.4-3658 LXB 18 08 27.58 -36 58 43.9           ~ 1051 0
24 X Sgr X-4 LXB 18 23 40.57 -30 21 40.6   19.06 18.81     ~ 1056 1
25 4U 1850-086 LXB 18 53 04.89 -08 42 19.7 20.40 21.20 21.0     ~ 266 1
26 4U 1857+01 LXB 19 08 26.97 +00 10 07.7 20.50 21.00 20.5     ~ 132 0
27 V* V1405 Aql LXB 19 18 47.6 -05 14 18 20.90 21.40 21.0     ~ 495 0
28 CXOU J212958.1+121002 XB* 21 29 58.06 +12 10 02.6     16.6     ~ 87 1

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