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Mean a465

This page presents lightcurves for Mean a465 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

This averaged lightcurve comes from a train of 24 bursts that can be viewed 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
modela465--Model ID
num24--Number of simulated bursts
z1.0%Metallicity mass fraction
h73.24%Hydrogen mass fraction
lAcc0.3--Accretion luminosity (1)
burstLength241.3 ± 9.0sBurst duration
peakLum10.33 ± 0.410+30WPeak lumonisity
persLum4.02 ± 0.1210+28WPersistent luminsoity
fluence5.66 ± 0.1410+32WFluence
tau54.8 ± 1.7sEquivalent burst duration (tau)
tDel0.98 ± 0.03hRecurrence time
conv4.81 ± 0.43%Convexity
r10905.328 ± 0.062s10% rise time
r25904.527 ± 0.046s25% rise time
singAlpha0.7 ± 0.01--Power law decay index
singDecay35.69 ± 3.11sExponential decay timescale
alpha38.4 ± 0.6--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