High resolution interferometry of astrophysical objects

dc.contributor.author	Raju, K. P
dc.date.accessioned	2007-05-04T10:40:54Z
dc.date.available	2007-05-04T10:40:54Z
dc.date.issued	1993
dc.identifier.citation	BASI, Vol. 21, pp. 373-374	en
dc.identifier.uri	http://hdl.handle.net/2248/1504
dc.description.abstract	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	en
dc.format.extent	152388 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Astrophysical objects	en
dc.subject	Thesis abstract	en
dc.title	High resolution interferometry of astrophysical objects	en
dc.type	Article	en