We study the presence of low intensity high velocity components, which we have termed wing features in the integrated Hα emission line profiles of the H II...
Expectations and Limits to Synthesize Nuclei with Z ≥ 120
In order to explore the possibilities to synthesize the new superheavy elements with Z=120, 122, 124, 126 some hot-fusion (mass asymmetric) reactions and cold...
Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View
We present a catalog of about 25,000 images of massive (M ⋆ ≥ 10 9 M ⊙) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for...
Expected Number of Massive Galaxy Relics in the Present Day Universe
The number of present day massive galaxies that have survived untouched since their formation at high-z is an important observational constraint to the...
Expected spectral characteristics of (101955) Bennu and (162173) Ryugu, targets of the OSIRIS-REx and Hayabusa2 missions
NASA's OSIRIS-REx and JAXA's Hayabusa2 sample-return missions are currently on their way to encounter primitive near-Earth asteroids (101955) Bennu and (162173)...
Experimental measurement of the quality factor of a Fabry-Pérot open-cavity axion haloscope
The axion is a hypothetical boson arising from the most natural solution to the problem of charge and parity symmetry in the strong nuclear force. Moreover...
Experimental validation of Lyot stop apodization in ground-based coronagraphy
We show that the use of apodizing functions at the coronagraph Lyot plane may be useful for improving the image contrast of ground-based coronagraphs. An...
Explaining the chemical trajectories of accreted and in-situ halo stars of the Milky Way
The Milky Way underwent its last significant merger ten billion years ago, when the Gaia-Enceladus-Sausage (GES) was accreted. Accreted GES stars and progenitor...
Explaining the Galactic Interstellar Dust Grain Size Distribution Function
We present here a new theoretical model designed to explain the interstellar dust grain size distribution function (IDGSDF), and compare its results with...