38 citations · 289 across the 24 of their papers we have counts for
26 papers
Speckle-interferometric study of close visual binary system Hip 11253 (HD14874) using Gaia (DR2) and (EDR3)
Hussam Aljboor, Ali Taani
We present a comprehensive set of physical and geometrical parameters for each of the components of the close visual binary system Hip 11253 (HD14874). We present an analysis for t…
Studying the age of supergiant companions in the magnetized X-ray binaries
Ali Taani
It has been proposed multiple times to use the neutron star (NS) in high-mass X-ray binaries (HMXBs) as an orbiting X-ray probe embedded in the wind-fed of its supergiant (SG) comp…
The binding energy produced within the framework of the accretion of millisecond pulsars
Ali Taani
The role and implication of binding energy through the accretion-induced collapse (AIC) of accreting white dwarfs (WDs) for the production of millisecond pulsars (MSPs) are investi…
Accretion-Induced Collapse of White Dwarfs as an Alternative Symbiotic Channel to Millisecond Pulsars
Ali Taani
Recently, extra motivation has been given to the investigations of an unresolved problem of millisecond pulsars (MSPs) produced by the recycling process, as an apparent role of the…
Assessing the complexity of orbital parameters after asymmetric kick in binary pulsars
Ali Taani, Juan C. Vallejo, Mohammed Abu-Saleem
The dynamical characterization of the Millisecond Pulsar (MSP) parameters is a key issue in understanding these systems. We present an analytical analysis of the orbital parameters…
Physical and geometrical parameters of CVBS XIV: The two nearby systems HIP 19206 and HIP 84425
Mashhoor A. Al-Wardat, Enas Abu-Alrob, Abdallah M. Hussein +6
The data release DR2 of Gaia mission was of great help in precise determination of fundamental parameters of Close Visual Binary and Multiple Systems (CVBMSs), especially masses of…
Metal-poor Stars Observed with the Automated Planet Finder Telescope. III. CEMP-no Stars are the Descendant of Population III Stars
Nour Aldein Almusleh, Ali Taani, Sergen Özdemir +4
In this study, we report a probabilistic insight into the stellar mass and supernovae (SNe) explosion energy of the possible progenitors of five CEMP-no stars. This was done by a d…
The Origin of LAMOST J1109+7459
Nour Aldein Almusleh, Yazan Khrais, Ali Taani
We report a comprehensive Chemo-dynamical analysis of LAMOST J1109+0754, a relatively bright (V = 12.8), extremely metal-poor ([Fe/H] = ), and prograde ( and $> 0…
Cosmological Insights into the Early Accretion of \textit{r}-Process-Enhanced stars. I. A Comprehensive Chemo-dynamical Analysis of LAMOST J1109+0754
Mohammad K. Mardini, Vinicius M. Placco, Yohai Meiron +10
This study presents a comprehensive chemo-dynamical analysis of LAMOST J1109+0754, a bright (V = 12.8), extremely metal-poor (\abund{Fe}{H} = ) star, with a strong \textit{r…
Probability Distribution of Magnetic Field Strengths through the Cyclotron Lines in High-Mass X-ray Binaries
Ali Taani, Awni Khasawneh, Mohammad Mardini +2
The study of variation of measured cyclotron lines is of fundamental importance to understand the physics of the accretion process in magnetized neutron star systems. We investigat…
Metal-poor Stars Observed with the Automated Planet Finder Telescope. II. Chemodynamical Analysis of Six Low-Metallicity Stars in the Halo System of the Milky Way
Mohammad K. Mardini, Vinicius M. Placco, Ali Taani +2
In this work, we study the chemical compositions and kinematic properties of six metal-poor stars with [Fe/H] in the Galactic halo. From high-resolution (R ~110,000)…
The Nucleosynthesis and Reaction Rates of Fluorine 19 () in the Sun
Mohammad K. Mardini, Nidal Ershiadat, Mashhoor A. Al-Wardat +4
We investigate the abundance of in the Sun through the nucleosynthesis scenario. In addition, we calculate the rate equations and reaction rates of the nucleosynthesis of…
Metal-poor stars observed with the automated planet finder telescope. I. Discovery of five carbon-enhanced metal-poor stars from LAMOST
Mohammad K. Mardini, Haining Li, Vinicius M. Placco +6
We report on the discovery of five carbon-enhanced metal-poor (CEMP) stars in the metallicity range of [Fe/H] . These stars were selected from the LAMOST DR3 low-res…
Stellar wind accretion and accretion disk formation: applications to neutron star high mass X-ray binaries
Shigeyuki Karino, Kenji Nakamura, Ali Taani
Recent X-ray observations have revealed the complexity and diversity of high-mass X-ray binaries (HMXBs). This diversity challenges a classical understanding of the accretion proce…
Probing the Accretion Induced Collapse of White Dwarfs in Millisecond Pulsars
Ali Taani, Awni Khasawneh
This paper investigates the progenitors of Millisecond Pulsars (MSPs) with a distribution of long orbital periods (P_orb > 2 d), to show the link between white dwarf (WD) binaries…
On the possibility of disk-fed formation in supergiant high-mass X-ray binaries
Ali Taani, Shigeyuki Karino, Liming Song +3
We have considered the existence of neutron star magnetic field given by the cyclotron lines. We collected the data of 9 sources of high-mass X-ray binaries with supergiant compani…
Determination of wind-fed model parameters of neutron stars in high-mass X-ray binaries
Ali Taani, Shigeyuki Karino, Liming Song +2
We have studied several neutron star high-mass X-ray binaries (HMXBs) with super-giant (SG) companions using a wind-fed binary model associated with the magnetic field. By using th…
Quiescent photometric modulations of two low-inclination cataclysmic variables KZGem and TWVir
Zhibin Dai, Paula Szkody, Ali Taani +2
The quiescent periodic photometric modulations of two low-inclination cataclysmic variables observed in Kepler K2 Campaigns 0 and 1, KZ Gem and TW Vir, are investigated. A phase-co…
Dynamical Monte Carlo Simulations of 3-D Galactic Systems in Axisymmetric and Triaxial Potentials
Ali Taani, Juan C. Vallejo
We describe the dynamical behavior of isolated old (> 1 G yr) objects-like Neutron Stars (NSs). These isolated NSs are evolved under smooth, time-independent, 3-D gravitational pot…
On the Distribution of Massive White Dwarfs and its Implication for Accretion-Induced Collapse
Ali Taani
A White Dwarf (WD) star and a main-sequence companion may interact through their different stellar evolution stages. This sort of binary population has historically helped us impro…
Evolution of Accreting Binary Systems on the Spin-up Line
Ali Taani, Mashhoor A. Al-Wardat, Awni Khasawneh
The measured characteristics of binary pulsars provide valuable insights into the evolution of these systems. We study the aspects of binary evolution particularly relevant to bina…
Impact of accretion on the statistics of neutron star masses
Z. Cheng, A. Taani, Y. H. Zhao
We have collected the parameter of 38 neutron stars (NSs) in binary systems with spin periods and measured masses. By adopting the Boot-strap method, we reproduced the procedure of…
Deriving fundamental parameters of millisecond pulsars via AIC in white dwarfs
A. Taani, Y. H. Zhao, A. Moraghan
We present a study of the observational properties of Millisecond Pulsars (MSPs) by way of their magnetic fields, spin periods and masses. These measurements are derived through th…
Modeling the Spatial Distribution of Neutron Stars in the Galaxy
Ali Taani, Luca Naso, Yingchun Wei +2
In this paper we investigate the space and velocity distributions of old neutron stars (aged 109 to 1010 yr) in our Galaxy. Galactic old Neutron Stars (NSs) population fills a toru…