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Model a351

This page presents lightcurves for Model a351 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
modela351--Model ID
num7--Number of simulated bursts
z0.4%Metallicity mass fraction
h74.9%Hydrogen mass fraction
lAcc0.03--Accretion luminosity (1)
burstLength113.2 ± 3.7sBurst duration
peakLum28.87 ± 0.6910+30WPeak lumonisity
persLum1.54 ± 0.0510+28WPersistent luminsoity
fluence8.96 ± 0.2110+32WFluence
tau31.0 ± 0.5sEquivalent burst duration (tau)
tDel18.15 ± 0.33hRecurrence time
conv9.5 ± 0.61%Convexity
r10905.084 ± 0.062s10% rise time
r25904.625 ± 0.032s25% rise time
singAlpha0.96 ± 0.01--Power law decay index
singDecay27.53 ± 1.92sExponential decay timescale
alpha45.8 ± 0.5--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