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[en] The structure of a slow reaction front on the surface of a dwarf, with a wake of escaping matter above it, is investigated. Simple expressions for all the important properties of such a front are given. It is found that a hydrogen or helium burning front is possible on a dwarf heavier than about one solar mass. For heavier fuels such a process seems impossible. (Auth.)
Journal
Astrophysics and Space Science; ISSN 0004-640X; 
; v. 60(1); p. 77-98
; v. 60(1); p. 77-98