Problem of the dynamic H II zone near the sun

Details Problem of the dynamic H II zone near the sun Problem of the dynamic H II zone near the sun

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sva....18..486a&link_type=abstract

(Astronomicheskii Zhurnal, vol. 51, July-Aug. 1974, p. 820-822.) Soviet Astronomy, vol. 18, Jan.-Feb. 1975, p. 486, 487. Transl

Astronomy and Astrophysics

Astronomy

Gas Ionization, Hydrogen Clouds, Interstellar Gas, Solar Activity Effects, Energy Distribution, Hydrogen Ions, Inelastic Collisions, Ion Temperature, Metastable State, Solar Radiation, Temperature Distribution

Scientific paper

Peculiar motions of the sun relative to the nearby interstellar gas are taken into account in a calculation of the ionization of this gas. When these motions are on the order of 20 km/sec, the sun forms an HII zone which is greatly extended in the direction of the antiapex. An influx of energy from individual acts of ionization and a loss of energy in the collisional excitation of metastable states and in charge exchanges determine the energy balance in this region. Electron and ion temperature distributions in the direction of the apex are obtained.

Affiliated with

Also associated with

No associations

Rating

Problem of the dynamic H II zone near the sun 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 Problem of the dynamic H II zone near the sun, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Problem of the dynamic H II zone near the sun will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1000618