Abstract
We present photo-ionization and morpho-kinematic analyses of the ejecta of novae. The sample consists of ten novae belonging to the Fe II, He/N and hybrid classes. The Fe II class of novae in the sample have bipolar cone-like structures, with or without equatorial rings with inclination angle in the range of 40◦–60◦. The He/N novae have bullet-nose curve along with bipolar cone-like structures and equatorial rings with an inclination angle of ∼80◦.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 225-229 |
| Number of pages | 5 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 15 |
| Issue number | 357 |
| DOIs | |
| State | Published - 2020 |
| Externally published | Yes |
| Event | 357th Symposium of the International Astronomical Union on White Dwarfs as Probes of Fundamental Physics: Tracers of Planetary, Stellar and Galactic Evolution - Hilo, United States Duration: Oct 21 2019 → Oct 25 2019 |
Keywords
- novae, cataclysmic variables
- stars: individual
- techniques: spectroscopic
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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