X-ray variability of sigma Orionis young stars with ROSAT
Abstract
We used the Aladin Virtual Obsrvatory tool and High Resolution Imager ROSAT archival data to search for X-ray variability in scale of days in 23 young stars in the sigma Orionis cluster and a background galaxy. Five stars displayed unambiguous flares and had probabilities p_var >> 99% of being actual variables. Two of the detected flares were violent and long-lasting, with maximum duration of six days and amplitude of eight times above the quiescent level. We classified another four stars as possible X-ray variables, including the binary system formed by the B2Vp star sigma Ori E and its close late-type companion. This makes a minimum frequency of high-amplitude X-ray variability in excess of a day of 39% among sigma Orionis stars. The incidence of this kind of X-ray variability seems to be lower among classical T Tauri stars with mid-infrared flux excesses than among fast-rotating, disk-less young stars.
Cite
@article{arxiv.0903.4814,
title = {X-ray variability of sigma Orionis young stars with ROSAT},
author = {J. A. Caballero and J. Lopez-Santiago and E. de Castro and M. Cornide},
journal= {arXiv preprint arXiv:0903.4814},
year = {2015}
}
Comments
AJ, in press