Fine Structure in H II Regions |
Contents
CHAPTER I | 11 |
CHAPTER II | 11 |
INTERFEROMETRY AND APERTURE SYNTHESIS | 11 |
2 other sections not shown
Common terms and phrases
Altenhoff amplitude and phase antenna aperture synthesis assumed Balick brightness temperature calibration Chapter Churchwell cocoon compact sources complex continuum cooling CORNELL LIBRARY CORNELL UNIVERSITY coverage delay patterns density distribution derived determined discussed dust e¹c early-type stars electron temperature emission measure equation equilibrium region estimate exciting star extended source fine structure flow model FLUX UNITS forbidden line frequencies fringe amplitude gion H II regions Hence Hjellming hour angle ionization front ionized gas km sec LIBRARY CORNELL LIBRARY UNIVERSITY line of sight lobe separation main sequence MAP CENTER Mezger neutral gas neutral region noise NRAO interferometer optical depth optically thin Orion nebula pc cm peak photons physical parameters plane point source possible present observations projected baselines protostars protostellar recombination line resolution resupply scale single-dish small structure stellar structure of H studies synthesis maps telescope Terzian thermal UNIVERSITY CORNELL velocity wavelengths X BAND