Filters
Results 1 - 1 of 1
Results 1 - 1 of 1.
Search took: 0.021 seconds
AbstractAbstract
[en] It is shown that at the stage when protostellar envelopes are blown away dense (n sub(e)>=10sup(7) cm sup(-3)) circumstellar ionized regions having radii r sub(H long)<=1014 cm are formed around stars with luminosities L < 104 Lsub(sun). These regions expand due to high Lysub(α) radiation pressure. Ultracompact (r sub(H long) approximately 1016 -1017 cm) H2 regions associated with OH maser sources are those which are formed around stars with Lsub(sun)>= 104 Lsub(sun). These objects display shell structure. At later stages compact H2 regions are formed
Original Title
Zarozhdenie i ehvolyutsiya oblastej ionizovannogo vodoroda v protsesse formirovaniya massivnykh zvezd
Primary Subject
Source
1985; 27 p; 27 refs.; 4 figs.
Record Type
Report
Report Number
Country of publication
Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue