The Collimation of Nonadiabatic Winds from Young Stars
نویسندگان
چکیده
منابع مشابه
Low Velocity Ionized Winds from Regions Around Young O Stars
We have observed seven ultracompact H II regions in hydrogen recombination lines in the millimeter band. Toward four of these regions, there is a high velocity (full width to half maximum 60–80 km s) component in the line profiles. The high velocity gas accounts for 35%–70% of the emission measure within the beam. We compare these objects to an additional seven similar sources we have found in ...
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ژورنال
عنوان ژورنال: International Astronomical Union Colloquium
سال: 1989
ISSN: 0252-9211
DOI: 10.1017/s025292110002385x