A dynamical study of the nova remnant of GK Per
Solar and Stellar Astrophysics
2013-10-17 v1
Abstract
Due to their large expansion speed, the apparent growth of nearby nova remnants such as GK Per can be easily resolved from ground-based optical imagery on a timescale of months. If the expansion in the plane of the sky is coupled with the Doppler shift velocities, an almost complete dynamical picture is drawn. We will discuss our latest results of such a study on GK Per.
Cite
@article{arxiv.1310.4488,
title = {A dynamical study of the nova remnant of GK Per},
author = {T. Liimets and R. L. M. Corradi and M. Santander-García and E. Villaver and P. Rodríguez-Gil and K. Verro and I. Kolka},
journal= {arXiv preprint arXiv:1310.4488},
year = {2013}
}
Comments
6 pages, 5 figures, to appear in Stella Novae: Past and Future Decades conference proceedings, P. A. Woudt & V. A. R. M. Ribeiro (eds), ASPCS