Skip to main content
Skip to main navigation menu
Skip to site footer
Open Menu
International Journal of Advanced Astronomy
About
About the Journal
Author Guidelines
Editorial Team
Indexing and Abstracting
Publication Ethics
Article Processing Charges
Current Issue
Archives
Submit a Manuscript
Other Journals
Contact us
Search
Register
Login
Home
/
Archives
/
Vol. 4 No. 1 (2016)
Vol. 4 No. 1 (2016)
Published:
2016-01-13
Articles
A general solution to non-collinear equilibria in terms of largest root (κ) of confocal oblate spheroid
M Javed Idrisi
1-4
Fractional action cosmology with an effective \(\wedge\) -term
Victor Shchigolev
5-10
Simple explanation for the ‘cosmological red-shift’ and it’s evidence
Hasmukh Tank
11-13
Stability of the equilibrium points in the circular restricted four body problem with oblate primary and variable mass
Abdullah Abduljabar Ansari
14-19
Quantum gravitational applications of nuclear, atomic and astrophysical phenomena
Satya Seshavatharam UV, Lakshminarayana S
20-26
Mach principle based explanation for the ‘cosmological red-shift’ and it’s evidence
Hasmukh K. Tank
27-28
Origin of dark mass apparentfrom gravitationally bound extended ordinary material systems
Shubhen Biswas
29-32
Stability of triangular equilibrium points in the Photogravitational elliptic restricted three body problem with Poynting-Robertson drag
Vivek Mishra, J.P. Sharma, Bhola Ishwar
33-38
Non-collinear libration points in CR3BP when less massive primary is an heterogeneous oblate body with N-layers
M Javed Idrisi, Kumari Shalini
39-42
Existence and stability of triangular points in the relativistic R3BP when the bigger primary is a triaxial rigid body and a source of radiation
Jagadish Singh, Bello Nakone
43-48
Existence and linear stability of triangular points in the perturbed relativistic R3BP when the bigger primary is an oblate spheroid
Bello Nakone, Jagadish Singh
49-56
Matter exhibiting absolute rest and the origin of the solar system
Daniel Robertson
57-60
Restricted three-body problem with stokes drag effect when less massive primary is an ellipsoid
M Javed Idrisi, Mamta Jain
61-67