High resolution interferometry of astrophysical objects

Details High resolution interferometry of astrophysical objects High resolution interferometry of astrophysical objects

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993basi...21..373r&link_type=abstract

Astronomical Society of India, Bulletin (ISSN 0304-9523), vol. 21, no. 3-4, p. 373-374

Other

Astronomical Interferometry, H Ii Regions, Orion Nebula, Solar Corona, Solar Magnetic Field, Stellar Spectrophotometry, Radial Velocity, Red Shift, Spectrum Analysis, Velocity Distribution

Scientific paper

The thesis comprises studies on two distinctly diverse astrophysical situations; one on the outer envelope of a late-type star at its main sequence stage (solar corona), the other on the ionized cloud surrounding an early-type star at its formation stage (the HII region -- Orion Nebula). The following problems are addressed in the work; the nature of velocity fields in the solar corona and its relations to local magnetic fields and the phase of the solar cycle, the excitation mechanism of the coronal green line and its variations in different coronal regions and the kinematics of an HII region in the farthest regions from the ionizing star.

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