Peculiarities of chemical and ionization equilibria in atmospheres of substars of solar elemental abundances at low temperatures

Details Peculiarities of chemical and ionization equilibria in atmospheres of substars of solar elemental abundances at low temperatures Peculiarities of chemical and ionization equilibria in atmospheres of substars of solar elemental abundances at low temperatures

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004kfnt...20..118k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 20, no. 2, p. 118-132

Computer Science

Scientific paper

A method of computing chemical equilibrium abundances through successive reaction adjustment in its Cruise version is adapted to treat ion and molecular abundances in gaseous system composed of Hydrogen and Helium with minor additives of second row elements. Equilibrium abundances with allowance for ionization have been studied in model atmospheres of cool substellar objects with solar elemental abundances with temperature of photosphere ca. 500--1500 K. Temperature and density dependencies as well as evolutionary trends are considered for abundances of individual species.

Affiliated with

Also associated with

No associations

Rating

Peculiarities of chemical and ionization equilibria in atmospheres of substars of solar elemental abundances at low temperatures 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 Peculiarities of chemical and ionization equilibria in atmospheres of substars of solar elemental abundances at low temperatures, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Peculiarities of chemical and ionization equilibria in atmospheres of substars of solar elemental abundances at low temperatures will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-736433