An atlas of models of H/+/ blisters

Details An atlas of models of H/+/ blisters An atlas of models of H/+/ blisters

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apjs...45..585i&link_type=abstract

Astrophysical Journal Supplement Series, vol. 45, Apr. 1981, p. 585-602. Research supported by the University of Minnesota

Astronomy and Astrophysics

Astrophysics

5

Astronomical Models, Early Stars, Hydrogen Clouds, Interstellar Gas, Ionized Gases, Stellar Evolution, Astronomical Maps, Density Distribution, Gas Density, Hydrogen Ions, Infrared Radiation, Mathematical Models, Nebulae, O Stars

Scientific paper

Early-type stars apparently form near the periphery of massive neutral clouds. The ionizing radiation of these stars interacts with the neutral gas and, because of the density gradient in the cloud, forms a blister of ionized gas. A sequence of models of these blisters is presented based on an earlier theoretical approximation of the transfer of the ionizing radiation. The models are presented as contour maps showing the predicted appearance of blisters around O5 V, O7 V, and O9 V stars in the 10-GHz radio and 30, 50, and 100 micron infrared bands. The characteristic systematic shift in the position of the emission maxima is again evident.

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