activity
20122024
most citedA new dynamical model for the study of galactic structure

32 citations · 132 across the 14 of their papers we have counts for

collaborators

14 papers

gr-qc2024

Behaviours of rip cosmological models in gravity

Amit Samaddar, S. Surendra Singh, Shah Muhammad +1

In this study, the Universe's rip cosmology theories have been provided for the gravity theory, where and stand for the non-metricity scalar and boundary term. We…

astro-ph.SR2024

Absolute dimensions of solar-type eclipsing binaries. NY Hya: A test for magnetic stellar evolution models

T. C. Hinse, O. Baştürk, J. Southworth +29

The binary star NY Hya is a bright, detached, double-lined eclipsing system with an orbital period of just under five days with two components each nearly identical to the Sun and…

astro-ph.GA201621 cited

Orbital and escape dynamics in barred galaxies - II. The 3D system: Exploring the role of the normally hyperbolic invariant manifolds

Christof Jung, Euaggelos E. Zotos

A three degrees of freedom (3-dof) barred galaxy model composed of a spherically symmetric nucleus, a bar, a flat disc and a spherically symmetric dark matter halo is used for inve…

astro-ph.GA20142 cited

Determining the nature of orbits in a three-dimensional galaxy model hosting a BL Lacertae object

Euaggelos E. Zotos

A three-dimensional dynamical model for a galaxy hosting a BL Lacertae object is constructed. The model consists of a logarithmic potential representing an elliptical host galaxy w…

astro-ph.GA201216 cited

Investigating the nature of motion in 3D perturbed elliptic oscillators displaying exact periodic orbits

Nicolaos D. Caranicolas, Euaggelos E. Zotos

We study the nature of motion in a 3D potential composed of perturbed elliptic oscillators. Our technique is to use the results obtained from the 2D potential in order to find the…

astro-ph.GA201229 cited

Trapped and escaping orbits in an axially symmetric galactic-type potential

Euaggelos E. Zotos

In the present article, we investigate the behavior of orbits in a time independent axially symmetric galactic type potential. This dynamical model can be considered to describe th…