The origin and evolution of multiple star systems
SSR Offner, M Moe, KM Kratter, SI Sadavoy… - arXiv preprint arXiv …, 2022 - arxiv.org
Observational advances over the last decade have enabled high-resolution, interferometric
studies of forming multiple systems, statistical surveys of multiplicity in star-forming regions …
studies of forming multiple systems, statistical surveys of multiplicity in star-forming regions …
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 …
within 150 pc of the Sun. It includes 27 young associations with ages in the range∼ 1–800 …
A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhood
CPM Bell, EE Mamajek, T Naylor - Monthly Notices of the Royal …, 2015 - academic.oup.com
We present a self-consistent, absolute isochronal age scale for young (≲ 200 Myr), nearby
(≲ 100 pc) moving groups in the solar neighbourhood based on homogeneous fitting of …
(≲ 100 pc) moving groups in the solar neighbourhood based on homogeneous fitting of …
[HTML][HTML] Dynamical traceback age of the β Pictoris moving group
Context. The β Pictoris moving group is one of the most well-known young associations in
the solar neighbourhood and several members are known to host circumstellar discs …
the solar neighbourhood and several members are known to host circumstellar discs …
CERES: a set of automated routines for echelle spectra
We present the Collection of Elemental Routines for Echelle Spectra (CERES). These
routines were developed for the construction of automated pipelines for the reduction …
routines were developed for the construction of automated pipelines for the reduction …
[HTML][HTML] The SPHERE infrared survey for exoplanets (SHINE)-I. Sample definition and target characterization
S Desidera, G Chauvin, M Bonavita, S Messina… - Astronomy & …, 2021 - aanda.org
Context. Large surveys with new-generation high-contrast imaging instruments are needed
to derive the frequency and properties of exoplanet populations with separations from~ 5 to …
to derive the frequency and properties of exoplanet populations with separations from~ 5 to …
Planet populations inferred from debris discs-Insights from 178 debris systems in the ISPY, LEECH, and LIStEN planet-hunting surveys
TD Pearce, R Launhardt, R Ostermann… - Astronomy & …, 2022 - aanda.org
We know little about the outermost exoplanets in planetary systems because our detection
methods are insensitive to moderate-mass planets on wide orbits. However, debris discs …
methods are insensitive to moderate-mass planets on wide orbits. However, debris discs …
Addressing systematics in the traceback age of the β Pictoris moving group
We characterize the impact of several sources of systematic errors on the computation of the
traceback age of the β Pictoris moving group (βPMG). We find that uncorrected gravitational …
traceback age of the β Pictoris moving group (βPMG). We find that uncorrected gravitational …
All-sky Co-moving Recovery Of Nearby Young Members (ACRONYM). II. The β Pictoris Moving Group∗
We confirm 66 low-mass stellar and brown dwarf systems (K7–M9) plus 19 visual or
spectroscopic companions of the β Pictoris moving group (BPMG). Of these, 41 are new …
spectroscopic companions of the β Pictoris moving group (BPMG). Of these, 41 are new …
ABUNDANCES IN THE LOCAL REGION. II. F, G, AND K DWARFS AND SUBGIANTS
RE Luck - The Astronomical Journal, 2016 - iopscience.iop.org
Parameters and abundances have been derived for 1002 stars of spectral types F, G, and K,
and luminosity classes IV and V. After culling the sample for rotational velocity and effective …
and luminosity classes IV and V. After culling the sample for rotational velocity and effective …