pith. sign in

arxiv: 1311.7618 · v1 · pith:EM7MLLW2new · submitted 2013-11-29 · 🌌 astro-ph.HE

Connection between orbital modulation of H-alpha and gamma-rays in the Be/X-ray binary LSI+61303

classification 🌌 astro-ph.HE
keywords fluxh-alphaorbitalfermi-latgamma-rayp-valueaverageband
0
0 comments X p. Extension
pith:EM7MLLW2 Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{EM7MLLW2}

Prints a linked pith:EM7MLLW2 badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

We studied the average orbital modulation of various parameters (gamma-ray flux, H-alpha emission line, optical V band brightness) of the radio- and gamma-ray emitting Be/X-ray binary LSI+61303. Using the Spearman rank correlation test, we found highly significant correlations between the orbital variability of the equivalent width of the blue hump of the H-alpha and Fermi-LAT flux with a Spearman p-value 2e-5, and the equivalent widths ratio EW_B/EW_R and Fermi-LAT flux with p-value 9e-5. We also found a significant anti-correlation between Fermi-LAT flux and V band magnitude with p-value 7.10^{-4}. All these correlations refer to the average orbital variability, and we conclude that the H-alpha and gamma-ray emission processes in LSI+61303 are connected. The possible physical scenario is briefly discussed.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.