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https://www.osti.gov/biblio/43...
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https://doi.org/10.2172/430865...
Report . 1974
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University of North Texas: UNT Digital Library
Report . 1974
Data sources: Bielefeld Academic Search Engine (BASE)
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Analytic pulsar models

descriptionPublicationkeyboard_double_arrow_right Report 16 Jan 1974 United States Publisher:Office of Scientific and Technical Information (OSTI)
Authors: Adams, R.C.; Cohen, J.M.; Adler, R.J.; Sheffield, C.;

doi: 10.2172/4308655

Analytic pulsar models

Abstract

An analytic and fully general relativistic solution to Einstein's field equations is given. This analytic model of a slowly rotating neutron star can describe differentially as well as uniformly rotating stars. (auth)

Country
United States
Related Organizations
Keywords

Radio & X-Ray Sources, Rotation, N56300* --Physics (Astrophysics & Cosmology)--Quasi-Stellar, Field Theories, *Neutron Stars-- Mathematical Models, *Pulsars-- Mathematical Models, 530, General Relativity Theory, 520

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average