Dynamical evolution of planetary nebulae

Details Dynamical evolution of planetary nebulae Dynamical evolution of planetary nebulae

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...153...79v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 153, no. 1, Dec. 1985, p. 79-90.

Astronomy and Astrophysics

Astrophysics

93

Interstellar Matter, Planetary Nebulae, Stellar Mass Ejection, Stellar Winds, Ionization, Radiant Cooling, Red Giant Stars, Wind Velocity

Scientific paper

The dynamical evolution of planetary nebulae is considered under the interacting-stellar-winds model. Analytical solutions to the dynamical equations are obtained assuming energy-conserving interaction. The authors have also investigated the effects of radiative cooling and the possible variation of the stellar wind from the central star. More realistic numerical calculations are performed taking into account the evolution of the central star using the model results of Schönberner (1983). The time dependences of the mass loss rate and velocity of the central-star wind is also included. The evolution of the ionization structure is obtained together with predictions of the evolution of X-ray and radio emissions from the nebulae.

Affiliated with

Also associated with

No associations

Rating

Dynamical evolution of planetary nebulae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dynamical evolution of planetary nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical evolution of planetary nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1159232