2004BaltA..13..116F

Query : 2004BaltA..13..116F

2004BaltA..13..116F - Baltic Astronomy, 13, 116-121 (2004/April-0)

Super-eddington winds of novae and other objects.

FRIEDJUNG M.

Abstract (from CDS):

The presence and physics of stellar winds, accelerated by radiation pressure in the continuum, is discussed for several types of objects, especially for classical novae. A luminosity above the Eddington limit is required for wind driving. This type of wind can be produced easily by a local rise in continuum opacity just after the critical point of the wind. It is possible to have other mechanisms, when the opacity does not rise above that due to Thomson scattering. Moreover, observational evidence exists indicating the reality of super-Eddington winds.

Abstract Copyright: ∼

Journal keyword(s): stars: novae, early type, Wolf-Rayet - stars: individual: η Car - stars: winds

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 LMCN 1988-10a No* 05 08 01.07 -68 37 37.5           ~ 38 0
3 OGLE 2016-NOVA-1 No* 05 09 58.3903831759 -71 39 52.714123608   16.0   17.0 17.38 ~ 87 0
4 LMCN 1990-01a No* 05 23 21.79 -69 29 48.4           ~ 61 0
5 LMCN 1988-03a No* 05 35 29.53 -70 21 30.9           ~ 51 0
6 * eta Car s*b 10 45 03.545808 -59 41 03.95124 6.37 7.03 6.48 6.123 4.41 LBV 2543 0
7 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
8 V* FH Ser No* 18 30 47.0401403328 +02 36 52.029761940           ~ 215 0

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