Structure of Radiative Shock Waves in Stellar Atmospheres

Details Structure of Radiative Shock Waves in Stellar Atmospheres Structure of Radiative Shock Waves in Stellar Atmospheres

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.260..127f&link_type=abstract

Astrophysics and Space Science, v. 260, Issue 1/2, p. 127-130 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

A global iteration method to determine the self-consistent structure of steady plane-parallel radiative shock waves is shown to converge to the stable solution with upstream front velocities of 15 km/s ≤ U 1≤ 60 km/s and for hydrogen gas of unperturbed temperature T= 3000 K and density ρ = 10-10gcm-3.

Affiliated with

Also associated with

No associations

Rating

Structure of Radiative Shock Waves in Stellar Atmospheres 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 Structure of Radiative Shock Waves in Stellar Atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure of Radiative Shock Waves in Stellar Atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1719905