2008ApJ...684..525C


Query : 2008ApJ...684..525C

2008ApJ...684..525C - Astrophys. J., 684, 525-531 (2008/September-1)

Damping of type I X-ray burst oscillations by convection.

COOPER R.L.

Abstract (from CDS):

I construct a simple model of the convective burning layer during a type I X-ray burst to investigate the effects convection has on the stability of the layer to nonradial oscillations. A linear perturbation analysis demonstrates that the region is stable to nonradial oscillations when energy transport is convection-dominated, but it is unstable when energy transport is radiation-dominated. Thus, efficient convection always dampens oscillations. These results may explain the nondetection of oscillations during the peak of some X-ray bursts.

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Journal keyword(s): Accretion, Accretion Disks - Stars: Neutron - X-Rays: Binaries - X-Rays: Bursts

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* V801 Ara LXB 16 40 55.5976953528 -53 45 04.948107156 17.50 18.20 17.5   17.07 ~ 921 0
2 NAME Slow Burster LXB 17 31 58.0 -33 49 58     15.50     ~ 865 1
3 SAX J1808.4-3658 LXB 18 08 27.58 -36 58 43.9           ~ 1051 0
4 V* V5511 Sgr LXB 18 13 39.03 -33 46 22.3   18.61 18.33 18.05   ~ 215 0
5 X Aql X-1 LXB 19 11 16.0571313336 +00 35 05.868232692           ~ 1186 1

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