NJ Wright - New Astronomy Reviews, 2020 - Elsevier
OB associations are unbound groups of young stars made prominent by their bright OB members, and have long been thought to be the expanded remnants of dense star clusters …
Context. In the last 15 years different ground-based spectroscopic surveys have been started (and completed) with the general aim of delivering stellar parameters and elemental …
A Kunder, G Kordopatis, M Steinmetz… - The Astronomical …, 2017 - iopscience.iop.org
ABSTRACT Data Release 5 (DR5) of the Radial Velocity Experiment (RAVE) is the fifth data release from a magnitude-limited ($9\lt I\lt 12$) survey of stars randomly selected in the …
C Soubiran, T Cantat-Gaudin… - Astronomy & …, 2018 - aanda.org
Context. Open clusters are very good tracers of the evolution of the Galactic disc. Thanks to Gaia, their kinematics can be investigated with an unprecedented precision and accuracy …
Context. Understanding how star formation begins and propagates through molecular clouds is a fundamental but still open question. One major difficulty in addressing this …
RMP Kerr, AC Rizzuto, AL Kraus… - The Astrophysical …, 2021 - iopscience.iop.org
Young stellar associations hold a star formation record that can persist for millions of years, revealing the progression of star formation long after the dispersal of the natal cloud. To …
E Zari, H Hashemi, AGA Brown, K Jardine… - Astronomy & …, 2018 - aanda.org
We study the three dimensional arrangement of young stars in the solar neighbourhood using the second release of the Gaia mission (Gaia DR2) and we provide a new, original …
Ages and masses of young stars are often estimated by comparing their luminosities and effective temperatures to pre-main-sequence stellar evolution tracks, but magnetic fields and …
Spectroscopy from the final internal data release of the Gaia–ESO Survey (GES) has been combined with Gaia EDR3 to assign membership probabilities to targets observed towards …