Recent Changes - Search:

PmWiki

pmwiki.org

edit SideBar

Model a187

This page presents lightcurves for Model a187 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
modela187--Model ID
num5--Number of simulated bursts
z1.0%Metallicity mass fraction
h73.24%Hydrogen mass fraction
lAcc1.11--Accretion luminosity (1)
burstLength220.7 ± 39.4sBurst duration
peakLum4.13 ± 0.210+30WPeak lumonisity
persLum15.53 ± 2.4910+28WPersistent luminsoity
fluence2.71 ± 0.5110+32WFluence
tau65.3 ± 10.5sEquivalent burst duration (tau)
tDel0.2 ± 0.01hRecurrence time
conv5.51 ± 1.53%Convexity
r10906.172 ± 0.103s10% rise time
r25904.914 ± 0.143s25% rise time
singAlpha0.5 ± 0.12--Power law decay index
singDecay24.59 ± 6.89sExponential decay timescale
alpha65.2 ± 7.5--Fluence ratio (alpha)
flag4--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

Back to the Index page

Edit - History - Print - Recent Changes - Search
Page last modified on December 21, 2015, at 06:57 PM