Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.290..317b&link_type=abstract
In ESA, Infrared Spectroscopy in Astronomy p 317-327 (SEE N90-19084 11-89)
Astronomy and Astrophysics
Astronomy
Cosmic Dust, Dwarf Novae, Infrared Astronomy, Infrared Spectroscopy, Symbiotic Stars, Emission Spectra, Infrared Spectra, Line Spectra, Molecules, Stellar Coronas, Stellar Spectra
Scientific paper
Infrared spectroscopy of classical, dwarf and recurrent novae, is reviewed. The impact of spectroscopy at wavelengths greater than 1 micron on the understanding of objects coming under the blanket title of novae and related stars is analyzed. The work includes the related class of symbiotic stars, some of which also undergo outbursts, and the central systems of which share some common characteristics with their cousins in the above group. Particular attention is paid to classical novae where infrared spectroscopy is invaluable in probing the early chemistry, formation of dust shells, and the origin of coronal line emission seen in many of these objects.
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