AG Pegasi - now a classical symbiotic star in outburst?
Solar and Stellar Astrophysics
2016-08-17 v1
Abstract
Optical spectroscopy study of the recent AG Peg outburst observed during the second half of 2015 is presented. Considerable variations of the intensity and the shape of the spectral features as well as the changes of the hot component parameters, caused by the outburst, are discussed and certain similarities between the outburst of AG Peg and the outburst of a classical symbiotic stars are shown. It seems that after the end of the symbiotic nova phase, AG Peg became a member of the classical symbiotic stars group.
Keywords
Cite
@article{arxiv.1608.02980,
title = {AG Pegasi - now a classical symbiotic star in outburst?},
author = {T. V. Tomov and K. A. Stoyanov and R. K. Zamanov},
journal= {arXiv preprint arXiv:1608.02980},
year = {2016}
}
Comments
8 pages, 6 figures, accepted by MNRAS