Monash X-ray burst wiki | Kepler / Model a367

This page presents lightcurves for Model a367 produced using the KEPLER simulation code, and analysed following Lampe, Heger & Galloway (2015).

The curve presented here is as measured in the neutron star's Newtonian rest frame. To compare this to an observation it is necessary to apply redshift corrections. Instructions for doing this are provided in the companion paper and a summary is provided here

An averaged representation of this burst train is available click here

Lightcurve

The mean luminosity (green line, left-hand y-axis), is plotted with the lighter green band giving the 1-sigma error calculated from the variation in the lightcurves included in the average. The radius is shown in blue (right-hand y-axis)

Parameters

The following table presents the initial conditions for the model and if a burst occurred, the average burst parameters.

Name	Value	Unit	Description
model	a367	--	Model ID
num	18	--	Number of simulated bursts
z	4.0	%	Metallicity mass fraction
h	64.96	%	Hydrogen mass fraction
lAcc	0.1	--	Accretion luminosity (1)
burstLength	47.7 ± 2.0	s	Burst duration
peakLum	21.55 ± 0.46	10+30W	Peak lumonisity
persLum	5.87 ± 0.15	10+28W	Persistent luminsoity
fluence	3.04 ± 0.06	10+32W	Fluence
tau	14.1 ± 0.2	s	Equivalent burst duration (tau)
tDel	2.29 ± 0.03	h	Recurrence time
conv	27.09 ± 1.74	%	Convexity
r1090	3.855 ± 0.204	s	10% rise time
r2590	3.631 ± 0.164	s	25% rise time
singAlpha	1.8 ± 0.21	--	Power law decay index
singDecay	6.83 ± 0.35	s	Exponential decay timescale
alpha	57.1 ± 1.3	--	Fluence ratio (alpha)
flag	2	--	Analysis quality flag (2)

(1) The accretion rate is in terms of the Eddington accretion rate $(1.75 \times 10^{-8} \, \mathrm{M}_\odot \, \mathrm{yr}^{-1})$

(2) Guide To Analyis Flags

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