106 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Chinese Academy of SciencesCN10 papers
- National Astronomical ObservatoriesCN8 papers
- GSI Helmholtz Centre for Heavy Ion ResearchDE6 papers
- Al al-Bayt UniversityJO5 papers
- Goethe University FrankfurtDE5 papers
- University of Chinese Academy of SciencesCN5 papers
- University of JordanJO5 papers
- University of Notre DameUS5 papers
- University of SharjahAE5 papers
- HUN-REN Institute for Nuclear ResearchHU4 papers
- Institute of Modern PhysicsCN3 papers
- Isra UniversityJO3 papers
10 papers · 1 filter
Gravitational Wave Strain and Orbital Dynamics of Binary Pulsars from LIGO-Virgo to LISA
Ali Taani
We summarize the current state of the art and calculate gravitational wave strain amplitudes for known binary pulsars, using data from current ground-based detectors (LIGO-Virgo-KA…
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…
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…
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…
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…