Numerical models of planetary nebulae evolution

Details Numerical models of planetary nebulae evolution Numerical models of planetary nebulae evolution

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...142..441o&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 142, no. 2, Jan. 1985, p. 441-450. Sponsorship: Deutsche Forschungsgemeinschaf

Statistics

Computation

54

Astronomical Models, Planetary Nebulae, Stellar Evolution, Computational Astrophysics, Cosmic Dust, Cosmic Gases, Hydrodynamic Equations, Ionization Potentials, Radiation Pressure, Stellar Mass Ejection, Stellar Winds

Scientific paper

Evolutionary sequences of planetary nebulae (PN) were calculated numerically beginning from the moment of PN envelope detachment to its dissipation. Gas and dust were treated as two separate hydrodynamical components and the equations for their motion were solved simultaneously with the frequency and angle dependent equations of radiation transfer in spherical symmetry. Radiation pressure on the dust component, the motion of the ionization front and the effect of a fast stellar wind were also included in the numerical calculations. Spectra of the outgoing radiation are presented for the infrared and radio frequency ranges. The general outline of PN evolution is discussed and comparisons with some observations are made.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-924597