2016A&A...591A..77S

Query : 2016A&A...591A..77S

2016A&A...591A..77S - Astronomy and Astrophysics, volume 591A77-77 (2016/7-1)

Non-linear behaviour of XTE J1550-564 during its 1998-1999 outburst, revealed by recurrence analysis.

SUKOVA P. and JANIUK A.

Abstract (from CDS):

We study the X-ray emission of the microquasar XTE J1550-564 and analyze the properties of its light curves using the recurrence analysis method. The indicators for non-linear dynamics of the accretion flow are found in the very high state and soft state of this source. The significance of deterministic variability depends on the energy band. We discuss the non-linear dynamics of the accretion flow in the context of the disc-corona geometry and propagating oscillations in the accretion flow.

Abstract Copyright: © ESO, 2016

Journal keyword(s): black hole physics - accretion, accretion disks - chaos

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 V* V381 Nor HXB 15 50 58.6637920704 -56 28 35.258385000           K3III 1254 0

Query : 2016A&A...591A..77S

Basic data :
V* V381 Nor -- High Mass X-ray Binary
Other object types: otypes_help 		X (2022MNRAS,XTE,...), gam (INTEGRAL1,INTREF), HXB (2016ApJS), V* (V*), * (Gaia)
ICRS coord. (ep=J2000) : 		15 50 58.6637920704 -56 28 35.258385000 (Optical) [ 1.4128 1.3058 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) : 		15 47 00.3325468289 -56 19 32.660061348 [ 1.4128 1.3058 90 ]
Gal coord. (ep=J2000) : 		325.8823100401135 -01.8268509670613 [ 1.4128 1.3058 90 ]
Proper motions mas/yr : 		-6.490 -3.490 [1.957 1.738 90] A 2020yCat.1350....0G
Parallaxes (mas): 		2.347 [2.5819] A 2020yCat.1350....0G
Spectral type: 		K3III D ~
Fluxes (1) :
G 20.810112 [0.017124] C 2020yCat.1350....0G
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Identifiers (7) :
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INTEGRAL1 17 V* V381 Nor [KRL2007b] 174 Gaia DR3 5884099221246440064
INTREF 660 XTE J1550-564 Gaia DR2 5884099221246440064

References (1254 between 1850 and 2026) (Total 1254)
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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Collections of Measurements Description of Measurements

Distance : 1    Plx : 1    PM : 1   

   

External archives :

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

Link by name to the catalogue in VizieR :

V* V381 Nor Gaia DR2 5884099221246440064 Gaia DR3 5884099221246440064

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