The spectral evolution of the slow nova V5558 Sgr has been monitored at the Loiano Observatory, Italy, during the pre-maximum stage and the early decline. The nova exhibited a long pre-maximum stage and several secondary outbursts after the initial maximum. The spectra during the pre-maximum stage s
β¦ LIBER β¦
The evolution of nova V5558 Sgr during the decline stage
β Scribed by R. Poggiani
- Publisher
- Elsevier Science
- Year
- 2010
- Tongue
- English
- Weight
- 552 KB
- Volume
- 15
- Category
- Article
- ISSN
- 1384-1076
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Spectral evolution of nova V5558 Sgr (no
β
R. Poggiani
π
Article
π
2008
π
Elsevier Science
π
English
β 318 KB
Evolution of the spectrum of Nova Androm
β
Huang Changchun; Chen Yafeng; Chen Ling
π
Article
π
1988
π
Elsevier Science
π
English
β 166 KB
The disc evolution of V2051 Oph on decli
β
Sonja Vrielmann; Warren Offutt
π
Article
π
2003
π
John Wiley and Sons
π
English
β 789 KB
The spectroscopic evolution of V459 Vul
β
R. Poggiani
π
Article
π
2010
π
Elsevier Science
π
English
β 472 KB
We report the spectroscopic follow-up of the nova V459 Vul carried out at the Loiano Observatory, Italy, at three epochs after the outburst. The spectroscopy showed high ionization lines of iron. The photometry has been used to estimate the absolute magnitude at maximum and the distance of the nova.
Sakurai's Object (V4334 Sgr): evolution
β
V. H. Tyne; A. Evans; T. R. Geballe; S. P. S. Eyres; B. Smalley; H. W. Duerbeck
π
Article
π
2002
π
John Wiley and Sons
π
English
β 393 KB
Optical and near-infrared observations o
β
S. Chaty; P. A. Charles; J. MartΓ; I. F. Mirabel; L. F. RodrΓguez; T. Shahbaz
π
Article
π
2003
π
John Wiley and Sons
π
English
β 249 KB