Titlebook: Regions of Recent Star Formation; Proceedings of the S R. S. Roger,Peter E. Dewdney Conference proceedings 1982 D. Reidel Publishing Compan

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Rheumatologist

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Conference proceedings 1982and photochemical effects in regions showing clear evidence of on-going star formation. This is currently an are a of considerable research activity with much new observational material over the wavelength range from X-ray to radio. Furthermore, the field isbeginning to mature. No longer is molecula

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A Multi-Purpose Scanning Fabry-Perot Interferometer System,mator/camera optics. A Fabry lens forms an image of the primary on the photocathode of a Ga-As PM tube. Scanning of the Fabry-Pérot and data acquisition is done by a dedicated Rockwell AIM 65 microcomputer soon to be replaced by a HP-85 equipped with the HP-IB IEEE 488 interface bus.

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0067-0057 dynamical and photochemical effects in regions showing clear evidence of on-going star formation. This is currently an are a of considerable research activity with much new observational material over the wavelength range from X-ray to radio. Furthermore, the field isbeginning to mature. No longer i

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HII Regions in Collapsing Massive Molecular Clouds,nted. Depending on the location of the exciting star, a champagne flow can occur concurrently with the central collapse of a nonrotating cloud. Partial evaporation of the cloud at a rate of about 0.005 M./yr results. When 100 0-stars are placed at the center of a freely falling cloud of 3 10. M. no

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The Dynamical Evolution of an HII Region, of models of star formation and HII region evolution. Strong evidence is found in support of the ‘champagne flow’ model of HII region evolution. There is no strong statistical evidence in support of the theory of successive star formation proposed by Elmegreen and Lada although there are several in

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Radio Continuum Observations of W1,at λ11cm using the 100-m telescope in both total power and polarized radiation. The central part of the object also has been observed with the Westerbork Synthesis Radio Telescope at λ49, λ21, and λ6cm. In the light of these observations, the question of the existence of a non-thermal component of W