3 citations · 4 across the 8 of their papers we have counts for
9 papers
Ensemble pulsational characteristics of eclipsing binaries containing Cep stars observed by the TESS mission
C. I. Eze, G. Handler, M. Vanrespaille +4
Massive pulsators in eclipsing binaries provide precise, model-independent stellar parameters that, combined with asteroseismic constraints, provide powerful probes of interior pro…
Orbital and stellar parameter determination of eclipsing Cep pulsators
C. I. Eze, G. Handler, F. Kahraman Aliçavuş +2
Eclipsing binaries provide precise constraints on stellar properties and evolution, making those hosting Cep pulsators particularly valuable for characterising massive pulsatin…
Characterizing the variability of a sample of massive stars in eclipsing binaries
C. I. Eze, G. Handler, F. Kahraman Aliçavuş +2
Massive stars exhibit a perplexing mismatch between their inferred masses from different observational techniques, posing a significant challenge to our understanding of stellar ev…
Eclipsing binary systems with Cephei components. V1216 Sco
A. Miszuda, C. I. Eze, F. Kahraman Alicavus +2
We present a detailed analysis of the high-mass binary system V1216 Sco, an eclipsing Algol-type binary hosting a Cephei pulsator, with an orbital period of 3.92 days. This sys…
Photometric sample of early B-type pulsators in eclipsing binaries observed with TESS
C. I. Eze, G. Handler
Asteroseismology coupled with eclipsing binary modelling shows a great potential in improving the efficiency of measurements or calibrations of the interior mixing profile in massi…
Cephei pulsators in eclipsing binaries observed with TESS
Christian I. Eze, Gerald Handler
The combined strength of asteroseismology and empirical stellar basic parameter determinations for in-depth asteroseismic analysis of massive pulsators in eclipsing binaries shows…
On the Evolution of Seyfert galaxies, BL Lacertae objects and Flat-spectrum radio quasars
Evaristus U. Iyida, Christian I. Eze, Finbarr C. Odo
The concept of the evolutionary sequence of jetted active galactic nuclei (AGNs) has been challenged in the last few decades since AGN subclasses are considered to be different due…
On the challenges of Angular Momentum Transfer Mechanism of Pulsar Glitches
I. O. Eya, C. I. Eze, E. U. Iyida
The angular momentum transfer mechanism of pulsar glitches for over four decades now stands as standalone theory with regards to glitch sizes and inter-glitch time intervals. Howev…
On the bimodal nature of the distributions of pulsar glitch sizes
I. O. Eya, E. U. Iyida, C. I. Eze
Pulsar glitches are sudden spin-ups in pulsar spin frequency (). The glitch size, , is a key parameter in any mechanism puts across towards the understanding of the events…