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Model a11

This page presents lightcurves for Model a11 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
modela11--Model ID
num13--Number of simulated bursts
z2.0%Metallicity mass fraction
h70.48%Hydrogen mass fraction
lAcc0.15--Accretion luminosity (1)
burstLength117.1 ± 5.7sBurst duration
peakLum17.77 ± 1.4510+30WPeak lumonisity
persLum4.17 ± 0.2110+28WPersistent luminsoity
fluence4.81 ± 0.110+32WFluence
tau27.2 ± 1.6sEquivalent burst duration (tau)
tDel2.96 ± 0.04hRecurrence time
conv10.91 ± 1.22%Convexity
r10905.111 ± 0.291s10% rise time
r25904.636 ± 0.358s25% rise time
singAlpha0.99 ± 0.07--Power law decay index
singDecay20.61 ± 2.81sExponential decay timescale
alpha69.1 ± 1.5--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