We present a high-resolution (R∼ 35 000), high signal-to-noise (S/N= 350) Magellan/MIKE
spectrum of the bright extremely metal-poor star 2MASS J1808− 5104. We find [Fe/H]=− 4.01 …

We present a chemo-dynamical analysis for 27 near main-sequence turnoff metal-poor
stars, including 20 stars analysed for the first time. The sample spans a range in [Fe/H] from …

We present the complete set of atmospheric and fundamental parameters, in addition to the
masses, for the individual components of eight stellar systems. The list of the systems …

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 of …

This study reports a probabilistic insight into the stellar‐mass and supernovae (SNe)
explosion energy of five CEMP‐no stars' possible progenitors. As such, a direct comparison …

As its periastron passage occurred during the third quarter of 2020, system 24 Aqr is of
particular significance. New visual solutions for the latest speckle interferometry …

The Milky Way is a spiral galaxy comprising three main components: the Bulge, the Disk,
and the Halo. Of particular interest is the Galactic disk, which holds a significant portion of …

In this paper, we investigate and define the topology of some astrophysical phenomena, like
the hairy (scalarized) charged black hole spacetime, to improve our understanding of the …

The dynamical interaction between binary systems is crucial in understanding the nature of
orbital motion under the influence of gravitational potential. In our study, we focused on …

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 …