Statistics – Computation
Scientific paper
Dec 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64.1233k&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Nov.-Dec. 1987, p. 1233-1242. In Russian.
Statistics
Computation
1
Chemical Equilibrium, Gas Dissociation, Hydrogen Ions, Molecular Ions, Neutron Stars, Stellar Magnetic Fields, Computational Astrophysics, Density Distribution, Gas Ionization, Stellar Temperature
Scientific paper
The equation of dissociative equilibrium for the molecular ion H2+ in a strong magnetic field B = 1012- 1013G is discussed. The equilibrium calculations are performed for the temperature region T ⪉ 2×106K. Ionization and dissociation balance is considered for the molecular ions H2+ and hydrogen atoms at total proton number desity Np= 1020- 1022cm-3. It is shown that when T ⪉ 2×105K, the major component of such a medium may be neutral hydrogen atoms. The number density of H2+ admixture can amount to 10-7 - 10-4 of the total proton density and depends on the magnetic field intensity and Np. Different spin modifications of H2+ in the total density of hydrogen molecular ions are also considered.
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