Line Evolution of the Nova V5587 Sgr from Early to Nebula Phase

Line Evolution of the Nova V5587 Sgr from Early to Nebula Phase

The spectral evolution of the nova V5587 Sgr has been monitored at Koyama Astronomical Observatory and Higashi-Hiroshima Observatory, Japan, from the early to nebula phase. The nova rebrightened several times. The spectra during the early phase showed emission lines of H α, H β, O I, He I, He II, N...

Full description

Saved in:
Bibliographic Details
Main Authors: T. Kajikawa, A. Arai, M. Nagashima, H. Kawakita, M. Yamanaka, K. Kawabata, S. Kiyota
Format: Article
Language:English
Published: Czech Technical University in Prague 2015-02-01
Series:Acta Polytechnica CTU Proceedings
Online Access:https://ojs.cvut.cz/ojs/index.php/APP/article/view/2908
Tags: Add Tag
No Tags, Be the first to tag this record!

Similar Items

Similar Items