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Spectroscopy of Novae -- A User's Manual
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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.
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Cited by 2 Pith papers
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The Unexplored Dusty Nova LMCN 2009-05a in the Large Magellanic Cloud
LMCN 2009-05a is a moderately fast D-class dusty nova in the LMC that formed carbonaceous dust around day 78, with a 700 K dust temperature on day 395 and a tcond-t2 point consistent with Galactic novae.
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Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation
Binary evolution modeling constrains donor masses of 14-23 solar masses for two luminous red novae and shows dust masses are 1-5 orders of magnitude below total ejected envelope masses.
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