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Model a30

This page presents lightcurves for Model a30 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.

NameValueUnitDescription
modela30--Model ID
num17--Number of simulated bursts
z0.1%Metallicity mass fraction
h75.9%Hydrogen mass fraction
lAcc0.082--Accretion luminosity (1)
burstLength309.1 ± 13.8sBurst duration
peakLum11.38 ± 0.7210+30WPeak lumonisity
persLum2.39 ± 0.1110+28WPersistent luminsoity
fluence7.45 ± 0.4510+32WFluence
tau65.5 ± 3.3sEquivalent burst duration (tau)
tDel4.77 ± 0.31hRecurrence time
conv2.96 ± 0.96%Convexity
r10905.134 ± 0.127s10% rise time
r25904.187 ± 0.074s25% rise time
singAlpha0.67 ± 0.01--Power law decay index
singDecay33.27 ± 3.57sExponential decay timescale
alpha39.3 ± 0.8--Fluence ratio (alpha)
flag0--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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Page last modified on December 21, 2015, at 06:57 PM