Disk Diffusion Propagation Model for the Outburst of XTE J1118+480

  • Wood K
  • Titarchuk L
  • Ray P
  • et al.
30Citations
Citations of this article
12Readers
Mendeley users who have this article in their library.

Abstract

We present a linear diffusion model for the evolution of the double-peaked outburst in the transient source XTE J1118+480. The model treats the two outbursts as episodic mass deposition at the outer radius of the disk followed by evolution of disk structure according to a diffusion process. We demonstrate that light curves with fast-rise, exponential decay profile are a general consequence of the diffusion process. Deconvolution of the light curve proves to be feasible and gives an input function specifying mass deposition at the outer disk edge as well as the total mass of the disk, both as functions of time. The derived evolution of total disk mass can be correlated with the observed evolution of the ~0.1 Hz QPO in the source reported by Wood et al.

Cite

CITATION STYLE

APA

Wood, K. S., Titarchuk, L., Ray, P. S., Wolff, M. T., Lovellette, M. N., & Bandyopadhyay, R. M. (2001). Disk Diffusion Propagation Model for the Outburst of XTE J1118+480. The Astrophysical Journal, 563(1), 246–254. https://doi.org/10.1086/323768

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free