Updated parameters of 1743 open clusters based on Gaia DR2

WS Dias, H Monteiro, A Moitinho… - Monthly Notices of …, 2021 - academic.oup.com
In this study, we follow up our recent paper (Monteiro et al.) and present a homogeneous
sample of fundamental parameters of open clusters in our Galaxy, entirely based on Gaia …

Fundamental parameters for 45 open clusters with Gaia DR2, an improved extinction correction and a metallicity gradient prior

H Monteiro, WS Dias, A Moitinho… - Monthly Notices of …, 2020 - academic.oup.com
Reliable fundamental parameters of open clusters (OCs) such as distance, age, and
extinction are key to our understanding of Galactic structure and stellar evolution. In this …

[HTML][HTML] A Gaia DR2 view of the open cluster population in the Milky Way

T Cantat-Gaudin, C Jordi, A Vallenari… - Astronomy & …, 2018 - aanda.org
Context. Open clusters are convenient probes of the structure and history of the Galactic
disk. They are also fundamental to stellar evolution studies. The second Gaia data release …

[HTML][HTML] Gaia data release 2-catalogue validation

F Arenou, X Luri, C Babusiaux, C Fabricius… - Astronomy & …, 2018 - aanda.org
Context. The second Gaia data release (DR2) contains very precise astrometric and
photometric properties for more than one billion sources, astrophysical parameters for …

BANYAN. XI. The BANYAN Σ multivariate Bayesian algorithm to identify members of young associations with 150 pc

J Gagné, EE Mamajek, L Malo, A Riedel… - The Astrophysical …, 2018 - iopscience.iop.org
BANYAN Σ is a new Bayesian algorithm to identify members of young stellar associations
within 150 pc of the Sun. It includes 27 young associations with ages in the range∼ 1–800 …

The Gaia-ESO Survey: revisiting the Li-rich giant problem

AR Casey, G Ruchti, T Masseron… - Monthly Notices of …, 2016 - academic.oup.com
The discovery of lithium-rich giants contradicts expectations from canonical stellar evolution.
Here we report on the serendipitous discovery of 20 Li-rich giants observed during the Gaia …

The 2014 ALMA long baseline campaign: first results from high angular resolution observations toward the HL Tau region

CL Brogan, LM Pérez, TR Hunter… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT We present Atacama Large Millimeter/submillimeter Array (ALMA) observations
from the 2014 Long Baseline Campaign in dust continuum and spectral line emission from …

[HTML][HTML] Gaia Early Data Release 3-Catalogue validation

C Fabricius, X Luri, F Arenou, C Babusiaux… - Astronomy & …, 2021 - aanda.org
Context. The third Gaia data release is published in two stages. The early part, Gaia EDR3,
gives very precise astrometric and photometric properties for nearly two billion sources …

Asymmetrical tidal tails of open star clusters: stars crossing their cluster's práh challenge Newtonian gravitation

P Kroupa, T Jerabkova, I Thies… - Monthly Notices of …, 2022 - academic.oup.com
After their birth a significant fraction of all stars pass through the tidal threshold (práh) of their
cluster of origin into the classical tidal tails. The asymmetry between the number of stars in …

[HTML][HTML] On the metallicity of open clusters-III. Homogenised sample

M Netopil, E Paunzen, U Heiter, C Soubiran - Astronomy & Astrophysics, 2016 - aanda.org
Context. Open clusters are known as excellent tools for various topics in Galactic research.
For example, they allow accurately tracing the chemical structure of the Galactic disc …