# 2000A&A...356..975K

 other querymodes : Identifierquery Coordinatequery Criteriaquery Referencequery Basicquery Scriptsubmission TAP Outputoptions Help

 Query : 2000A&A...356..975K

2000A&A...356..975K - Astronomy and Astrophysics, volume 356, 975-988 (2000/4-3)

Internal shock model for microquasars.

KAISER C.R., SUNYAEV R. and SPRUIT H.C.

Abstract (from CDS):

We present a model for the radio outbursts of microquasars based on the assumption of quasi-continuous jet ejection. The jets are lit up' by shock fronts traveling along the jets during outbursts. The shocks accelerate relativistic particles which emit the observed synchrotron radiation. The observed comparatively flat decay light curves combined with gradually steepening spectral slopes are explained by a superposition of the radiation of the aging relativistic particle population left behind by the shocks. This scenario is the low energy, time-resolved equivalent to the internal shock model for GRBs. We show that this model predicts energy contents of the radiating plasma similar to the plasmon model. At the same time, the jet model relaxes the severe requirements on the central source in terms of the rate at which this energy must be supplied to the jet. Observations of mini-bursts' with flat spectral slopes and of infrared emission far from the source centre suggest two different states of jet ejections: (i) A `mini-burst' mode with relatively stable jet production and weak radio emission with flat spectra and (ii) an outburst mode with strong variations in the jet bulk velocities coupled with strong radio emission with steeper spectra. We also show that the continuous jets in microquasars should terminate in strong shocks and possibly inflate radio lobes similar to extragalactic jet sources. We investigate the possibility of testing the predictions of this model with resolved radio observations. Finally, we suggest that Doppler-shifted X-ray iron lines, and possibly H-α lines, may be emitted by the jet flow of microquasars if thermal instabilities analogous to those in SS 433 exist in their jets.

Journal keyword(s): shock waves - stars: binaries: general - stars: individual: GRS 1915+105 - radio continuum: stars

 Number of rows : 7
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 V* V1033 Sco HXB 16 54 00.137 -39 50 44.90   15.20 14.2 16.14   F5IV 1793 1
2 NAME Great Annihilator LXB 17 43 54.83 -29 44 42.6           ~ 658 1
3 AX J1748.0-2829 LXB 17 48 05.060 -28 28 25.80     13.60     ~ 179 0
4 2XMM J180112.4-254436 LXB 18 01 12.40 -25 44 36.1           ~ 374 1
5 SS 433 HXB 19 11 49.5647697480 +04 58 57.827127648   16.3 13.0     A7Ib: 2028 4
6 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2454 0
7 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4122 0

To bookmark this query, right click on this link: simbad:objects in 2000A&A...356..975K and select 'bookmark this link' or equivalent in the popup menu

2022.08.14-11:24:58