Continuum emission from classical nova winds

Details Continuum emission from classical nova winds Continuum emission from classical nova winds

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204...45h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, July 1983, p. 45-52. Research supported by the Sci

Astronomy and Astrophysics

Astronomy

7

Continuous Radiation, Novae, Stellar Radiation, Stellar Winds, Black Body Radiation, Photosphere, Radiative Transfer, Stellar Models

Scientific paper

The emergent continuum of a slow classical nova during outburst is studied using the quasi-steady optically thick, transonic wind models of Ruggles and Bath (1979). Models are developed for various steady mass loss rates and these models are then related to the evolution of slow novae during decline and early post-maximum. It is shown that the continuum emission departs radically from a blackbody spectrum and exhibits features common to highly extended stellar atmospheres.

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