collaborators

6 papers

astro-ph.GA2026

Galaxy interactions in void substructures: Morphology and stellar populations of two triplets from CAVITY

G. M. Azevedo, A. L. Chies-Santos, R. Riffel +5

Context. Cosmic voids are underdense regions of the Universe that provide a unique environment to study galaxy evolution in relative isolation. Galaxy triplets in voids are rare sy…

astro-ph.GA2025

The Milky Way in motion: gauging stellar trajectories that shape the Galactic thin disc

M. L. L. Dantas, R. Smiljanic, R. S. de Souza +2

As stars traverse the Milky Way, their orbits evolve through perturbations that alter their orbital radii. These changes arise from two mechanisms: churning, which modifies angular…

astro-ph.GA2025

The low-mass and structured stellar halo of M83 argues against a merger origin for its starburst and extended neutral hydrogen disk

Eric F. Bell, Benjamin Harmsen, Matthew Cosby +12

A merger origin has been suggested for M83's massive, metal-rich extended HI disk and nuclear starburst. We observe M83's stellar halo to test this idea. We train nearest-neighbor…

astro-ph.GA2025

An ALMA Band 7 survey of SDSS/Herschel quasars in Stripe 82: I. The properties of the 870 micron counterparts

E. Hatziminaoglou, H. Messias, R. Souza +6

(Abridged) Quasar studies with Herschel/SPIRE often report host luminosities ranging from 10^{12} to 10^{14} Lsun, suggestive of star formation rates (SFRs) of up to several thousa…

astro-ph.SR2025

Probing the origins. II. Unravelling lithium depletion and stellar motion: Intrinsic stellar properties drive depletion, not kinematics

M. L. L. Dantas, R. Smiljanic, D. Romano +4

In Paper I, we classified a stellar sample from the thin disc with a broad range in metallicity as being churned outward or inward, or blurred/undisturbed. In this paper (Paper II)…

astro-ph.GA2025

Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity

M. L. L. Dantas, R. Smiljanic, R. S. de Souza +2

We employ a Generalised Additive Model (GAM) to address the limitations inherent in radial metallicity gradients predicted by chemical evolution models, thereby facilitating the es…