pith. sign in

arxiv: 1402.7168 · v1 · pith:IFHJRU7Tnew · submitted 2014-02-28 · 🌌 astro-ph.SR

On the incidence of eclipsing Am binary systems in the SuperWASP survey

classification 🌌 astro-ph.SR
keywords systemseclipsingstarseclipsesfoundidentifiedpresentedsuperwasp
0
0 comments X p. Extension
pith:IFHJRU7T Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{IFHJRU7T}

Prints a linked pith:IFHJRU7T badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analysed for the presences of eclipses. A total of 70 stars were found to exhibit eclipses, with 66 having sufficient observations to enable orbital periods to be determined and 28 of which are newly identified eclipsing systems. Also presented are spectroscopic orbits for 5 of the systems. The number of systems and the period distribution is found to be consistent with that identified in previous radial velocity surveys of `classical' Am stars.

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.