output
20042026
most citedMulti-Element Abundance Measurements from Medium-Resolution Spectra. III. Metallicity Distributions of Milky Way Dwarf Satellite Galaxies

336 citations

Showing 2023Show all

6 papers · 1 filter

hep-ph2023★ 6 cited

Kaon Structure in the Nuclear Medium within the Light Front Approach

G. H. S. O. Yabusaki, J. P. B. C. de Melo, K. Tsushima +2

We study the properties of the charged kaon in symmetric nuclear matter using a Bethe-Salpeter amplitude to model the quark-anti-quark bound state, which is well constrained by pre…

hep-ph2023★ 3 cited

Pseudoscalar current and covariance with the light-front approach

Jurandi Leãoo, J. P. B. C. de Melo

Quantum Field Theory (QFT) is used to describe the physics of particles in terms of their fundamental constituents. The Light-Front Field Theory~(LFFT), introduced by Paul Dirac in…

hep-ph2023★ 1 cited

Covariant form factors for spin-1 particles

J. P. B. C. de Melo

Spin-1 particles, is a fundamental bound state for the two quarks, and play a crucial role in elucidating the electromagnetic properties within the realm of hadronic physics. Their…

astro-ph.SR2023★ 9 cited

The cosmic waltz of Coma Berenices and Latyshev 2 (Group X). Membership, phase-space structure, mass, and energy distributions

J. Olivares, N. Lodieu, V. J. S. Béjar +3

Context. Open clusters (OCs) are fundamental benchmarks where theories of star formation and stellar evolution can be tested and validated. Coma Ber and Latyshev 2 (Group X) are th…

astro-ph.SR2023★ 22 cited

Dynamical age of the Tucana-Horologium young stellar association

Phillip A. B. Galli, Núria Miret-Roig, Hervé Bouy +2

The Tucana-Horologium association is one of the closest young stellar groups to the Sun and despite the close proximity its age is still debated in the literature. We take advantag…

astro-ph.GA2023★ 3 cited

Boundary conditions in hydrodynamic simulations of isolated galaxies and their impact on the gas-loss processes

Anderson Caproni, Gustavo A. Lanfranchi, Amâncio C. S. Friaça +1

Three-dimensional hydrodynamic simulations are commonly used to study the evolution of the gaseous content in isolated galaxies, besides its connection with galactic star formation…