SS 433: Stationary lines and primary eclipses
Solar and Stellar Astrophysics
2015-10-14 v1
Abstract
Some stationary lines in the emission spectra of SS 433 are eclipsed, but most are not. Lines attributed to a circumbinary disk are not eclipsed, but double in relative intensity during primary eclipse. A C II doublet is eclipsed and Doppler shifts over two periods yield an orbital speed of 176 +/- 13 km/s.
Cite
@article{arxiv.1510.03667,
title = {SS 433: Stationary lines and primary eclipses},
author = {M. G. Bowler},
journal= {arXiv preprint arXiv:1510.03667},
year = {2015}
}
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