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...
Main Authors: | T. Kajikawa, A. Arai, M. Nagashima, H. Kawakita, M. Yamanaka, K. Kawabata, S. Kiyota |
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Format: | Article |
Language: | English |
Published: |
CTU Central Library
2015-02-01
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Series: | Acta Polytechnica CTU Proceedings |
Online Access: | https://ojs.cvut.cz/ojs/index.php/APP/article/view/2908 |
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