The surface chemistry of stars. I - Diffusion of heavy ions in white dwarf envelopes. II - Fractionated accretion of interstellar matter

Details The surface chemistry of stars. I - Diffusion of heavy ions in white dwarf envelopes. II - Fractionated accretion of interstellar matter The surface chemistry of stars. I - Diffusion of heavy ions in white dwarf envelopes. II - Fractionated accretion of interstellar matter

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235..534a&link_type=abstract

Astrophysical Journal, Part 1, vol. 235, Jan. 15, 1980, p. 534-553.

Physics

108

Ionic Diffusion, Stellar Atmospheres, Stellar Envelopes, Stellar Mass Accretion, Surface Reactions, White Dwarf Stars, Abundance, Gas Ionization, Gravitational Effects, Heavy Ions, Interstellar Gas, Stellar Evolution, Stellar Winds, Trace Elements

Scientific paper

The diffusion separation of heavy elements in the envelopes of white
dwarfs is examined. Consideration is given to the physics of diffusion
with particular reference to the conditions in white dwarfs. A solution
of the diffusion equation that includes the effects of convection and
accretion is presented.

Affiliated with

Also associated with

No associations

Rating

The surface chemistry of stars. I - Diffusion of heavy ions in white dwarf envelopes. II - Fractionated accretion of interstellar matter 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 The surface chemistry of stars. I - Diffusion of heavy ions in white dwarf envelopes. II - Fractionated accretion of interstellar matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The surface chemistry of stars. I - Diffusion of heavy ions in white dwarf envelopes. II - Fractionated accretion of interstellar matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-880685