collaborators

5 papers

astro-ph.GA2026

A new Gaia census of OB associations within 1 kpc

Alexis L. Quintana, Nicholas J. Wright, Lilly A. Kormann +6

OB associations are primordial tracers of star formation and Galactic structure. Originally defined about 80 years ago, their historical membership lists have been superseded thank…

astro-ph.SR2026

Re-visiting the Canis Major star-forming region with Gaia data release 3 data

S. Nogueira-Silva, P. A. B. Galli, J. Olivares +7

Context: The Canis Major (CMa) star-forming region, a remote molecular cloud complex within the recently discovered Radcliffe Wave, remains under-explored in the literature. Aims:…

astro-ph.GA2025

The late Miocene Be anomaly and the possibility of a supernova

E. Maconi, J. Alves, J. Großschedl +3

Recent measurements of cosmogenic Be in deep-ocean ferromanganese crusts from the Central and Northern Pacific have revealed an anomalous concentration between 11.5 and 9.0…

astro-ph.GA2025

The Solar System's passage through the Radcliffe wave during the middle Miocene

E. Maconi, J. Alves, C. Swiggum +14

Context. As the Solar System orbits the Milky Way, it encounters various Galactic environments, including dense regions of the interstellar medium (ISM). These encounters can compr…

astro-ph.SR2025

The TW Hydrae Association is a cluster chain of Sco-Cen

N. Miret-Roig, J. Alves, S. Ratzenböck +9

The TW Hydrae Association (TWA) is a young local association (YLA) about 50 pc from the Sun, offering a unique opportunity to study star and planet formation processes in detail. W…