Oscillations of differentially rotating and tidally distorted gaseous spheres : Effect of non-uniform density-Reference-Cited by-同舟云学术

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Oscillations of differentially rotating and tidally distorted gaseous spheres : Effect of non-uniform density

Published:2021-10 Issue: Volume:88 Page:101612
ISSN:1384-1076
Container-title:New Astronomy
language:en
Short-container-title:New Astronomy

Author:

Kumar Sunil^ORCID,Saini Seema,Singh Kamal Krishan,Bhatt Vineet,Mohan Chander

Funder

Sharda University

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics,Instrumentation

Reference31 articles.

1. Surface effects in main-sequence solar-like oscillators computed using three-dimensional radiation hydrodynamics simulations;Ball;Astronomy & Astrophysics,2016

2. Solar p-mode eigenfrequencies are decreased by turbulent convection;Brown;Science,1984

3. Dynamical instability of gaseous masses approaching the schwarzschild limit in general relativity;Chandrasekhar;Phys. Rev. Lett.,1964

4. The dynamical instability of gaseous masses approaching the schwarzschild limit in general relativity;Chandrasekhar;Astrophys. J.,1964

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Small adiabatic barotropic non-radial modes of oscillations of differentially rotating stars;INTERNATIONAL SCIENTIFIC AND PRACTICAL CONFERENCE “TECHNOLOGY IN AGRICULTURE, ENERGY AND ECOLOGY” (TAEE2022);2022

2. A mathematical approach of determining radial oscillations of differentially rotating polytropic stars;INTERNATIONAL SCIENTIFIC AND PRACTICAL CONFERENCE “TECHNOLOGY IN AGRICULTURE, ENERGY AND ECOLOGY” (TAEE2022);2022

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