Spectroscopy of Novae -- A User's Manual
arXiv:1211.3176
Abstract
The spectroscopic development of classical novae is described as a narrative of the various stages of the outburst. The review highlights the multiwavelength aspects of the phenomenology and the recent developments related to structure, inhomogeneity, and dynamics of the ejecta. Special emphasis is placed on the distinct behavior of the symbiotic-like recurrent novae.
Invited review article 2012 in Bulletin of the Astronomical Society of India (BASI), 28 pages, 17 figs
Cited by in corpus (8)
- Fermi Establishes Classical Novae as a Distinct Class of Gamma-Ray Sources
- Observations of Galactic and Extragalactic Novae
- Radiative shocks create environments for dust formation in novae
- Novae as Tevatrons: Prospects for CTA and IceCube
- On a century of extragalactic novae and the rise of the rapid recurrent novae
- Beryllium detection in the very fast nova ASASSN-16kt (V407 Lupi)
- Shocks in nova outflows. II. Synchrotron radio emission
- Broad absorption line symbiotic stars: highly ionized species in the fast outflow from MWC 560