Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars - Error-removing techniques

Details Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars - Error-removing techniques Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars - Error-removing techniques

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.126..119g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 126, no. 1, Oct. 1986, p. 119-132.

Astronomy and Astrophysics

Astrophysics

6

Perturbation Theory, Polytropic Processes, Stellar Models, Stellar Rotation, Error Analysis, Numerical Integration

Scientific paper

In this paper we analyse error-removing techniques used without
sufficient theoretical support in a previous paper, where
Chandrasekhar's higher-order perturbation theories were developed for
either uniformly or differentially-rotating polytropic stars

Affiliated with

Also associated with

No associations

Rating

Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars - Error-removing techniques does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars - Error-removing techniques, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars - Error-removing techniques will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1735508