ISO observations of classical novae: Preliminary analysis and results

A. Salama, P. Barr, J. Clavel, K. Leech, M. F. Kessler, T. Lim, L. Metcalfe, B. Schulz, S. P.S. Eyres, R. N. Jenkins, A. Evans

Allbwn ymchwil: Cyfraniad at gyfnodolynErthygladolygiad gan gymheiriaid

2 Dyfyniadau (Scopus)

Crynodeb

We describe the ISO programme to observe classical novae. The programme includes observations of novae during and shortly after eruption, and old novae. ISO observations of far infrared fine structure lines are providing us with information about physical conditions in nova ejecta which complement and extend knowledge obtained from ground-based observations. Surprisingly, we are getting little information about dust in nova systems, despite the fact that many novae are prolific dust-producers.

Iaith wreiddiolSaesneg
Tudalennau (o-i)227-235
Nifer y tudalennau9
CyfnodolynAstrophysics and Space Science
Cyfrol255
Rhif cyhoeddi1-2
Dynodwyr Gwrthrych Digidol (DOIs)
StatwsCyhoeddwyd - 1997

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