Stellar variability in Gaia DR3-I. Three-band photometric dispersions for 145 million sources

JM Apellániz, G Holgado, MP González… - Astronomy & …, 2023 - aanda.org
Context. The unparalleled characteristics of Gaia photometry in terms of calibration, stability,
time span, dynamic range, full-sky coverage, and complementary information make it an …

Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A

T Ansín, R Gamen, NI Morrell, RH Barba… - Monthly Notices of …, 2023 - academic.oup.com
The evolution of massive stars is not completely understood. Several phenomena affect their
birth, life, and death, multiplicity being one of them. In this context, the OWN and MONOS …

The population of young low-mass stars in Trumpler 14

D Itrich, L Testi, G Beccari, CF Manara, M Reiter… - Astronomy & …, 2024 - aanda.org
Massive star-forming regions are thought to be the most common birth environments in the
Galaxy and the only birth places of very massive stars. Their presence in the stellar cluster …

Into the Mystic: ALMA ACA observations of the Mystic Mountains in Carina

M Reiter, PD Klaassen, L Moser-Fischer… - Monthly Notices of …, 2023 - academic.oup.com
We present new observations of the Mystic Mountains cloud complex in the Carina Nebula
using the ALMA Atacama Compact Array (ACA) to quantify the impact of strong UV radiation …

Extinction, the elephant in the room that hinders optical Galactic observations

JM Apellániz - arXiv preprint arXiv:2401.01116, 2024 - arxiv.org
Extinction is the elephant in the room that almost everyone tries to avoid when analyzing
optical/IR data: astronomers tend to find a quick fix for it that the referee will accept, but that …

[PDF][PDF] Probing particle acceleration in stellar binary systems using gamma-ray observations

J Hinton - inspirehep.net
Only a few gamma-ray sources have been established as proton accelerators over the last
decades, among them two extraordinary binary systems, the massive colliding wind binary …