Flow near the critical line in a gasdynamic model of stellar wind with heat conduction

Details Flow near the critical line in a gasdynamic model of stellar wind with heat conduction Flow near the critical line in a gasdynamic model of stellar wind with heat conduction

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993primm..57..156s&link_type=abstract

Prikladnaya Matematika i Mekhanika (ISSN 0032-8235), vol. 57, no. 3, p. 156-160.

Physics

Conductive Heat Transfer, Gas Dynamics, Hydrodynamic Equations, Stellar Winds, Stellar Atmospheres, Stellar Models, Supersonic Flow

Scientific paper

A one-dimensional stationary spherical symmetric model of stellar wind is examined within the framework of gas dynamics assuming that energy transfer in the outer atmosphere of a star is realized through electron heat conduction. The shape of the critical curve corresponding to the subsonic-supersonic transition is investigated in detail; the types of the singular points on the curve and their relation to the separatrix directions are examined. The stability of the solutions with respect to perturbations in the vicinity of singular points is analyzed using the approach proposed by Kulikovskii and Slobodkina (1967).

Affiliated with

Also associated with

No associations

Rating

Flow near the critical line in a gasdynamic model of stellar wind with heat conduction 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 Flow near the critical line in a gasdynamic model of stellar wind with heat conduction, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Flow near the critical line in a gasdynamic model of stellar wind with heat conduction will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1336357