A dynamical study of the nova remnant of GK Per

Дата и время публикации : 2013-10-16T19:51:48Z

Авторы публикации и институты :
T. Liimets
R. L. M. Corradi
M. Santander-García
E. Villaver
P. Rodríguez-Gil
K. Verro
I. Kolka

Ссылка на журнал-издание: Ссылка на журнал-издание не найдена
Коментарии к cтатье: 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
Первичная категория: astro-ph.SR

Все категории : astro-ph.SR

Краткий обзор статьи: 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.

Category: Physics