Supercritical winds from cool 'canonical' stars caused by evolution on the main sequence

dc.contributor.author	Venkatakrishnan, P
dc.date.accessioned	2009-01-28T12:35:56Z
dc.date.available	2009-01-28T12:35:56Z
dc.date.issued	1986-02
dc.identifier.citation	Astrophysics and Space Science, Vol. 119, No. 1, pp. 51 - 55	en
dc.identifier.issn	0004-640X
dc.identifier.uri	http://hdl.handle.net/2248/4290
dc.description.abstract	Even the very slow expansion of a star's radius due to evolution on the Main Sequence is shown to be supercritical for cool stars without coronae. Since steady sphericaily-symmetric supercitical solutions are theoretically impossible, unsteady supercritical solutions are studied. It is seen that smooth sonic transitions are possible in the unsteady case, but are accompanied by enhancement of pressure over the critical values.	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Co.	en
dc.relation.uri	http://www.springerlink.com/content/g71277m182361k07/	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1986Ap%26SS.119...51V	en
dc.subject	Cool Stars	en
dc.subject	Main Sequence Stars	en
dc.subject	Stellar Evolution	en
dc.subject	Stellar Winds	en
dc.subject	Supercritical Flow	en
dc.subject	Acoustic Velocity	en
dc.subject	Computational Astrophysics	en
dc.subject	Radii	en
dc.subject	Stellar Temperature	en
dc.subject	Unsteady Flow	en
dc.title	Supercritical winds from cool 'canonical' stars caused by evolution on the main sequence	en
dc.type	Article	en