Young stars near the sun

B Zuckerman, I Song - Annu. Rev. Astron. Astrophys., 2004 - annualreviews.org
▪ Abstract Until the late 1990s the rich Hyades and the sparse UMa clusters were the only
coeval, comoving concentrations of stars known within 60 pc of Earth. Both are hundreds of …

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 active lives of stars: a complete description of the rotation and XUV evolution of F, G, K, and M dwarfs

CP Johnstone, M Bartel, M Güdel - Astronomy & Astrophysics, 2021 - aanda.org
Aims. We study the evolution of the rotation and the high energy X-ray, extreme ultraviolet
(EUV), and Ly-α emission for F, G, K, and M dwarfs, with masses between 0.1 and 1.2 M⊙ …

CARMENES input catalogue of M dwarfs-V. Luminosities, colours, and spectral energy distributions

C Cifuentes, JA Caballero, M Cortés-Contreras… - Astronomy & …, 2020 - aanda.org
Context. The relevance of M dwarfs in the search for potentially habitable Earth-sized
planets has grown significantly in the last years. Aims. In our on-going effort to …

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 …

The apache point observatory galactic evolution experiment (APOGEE)

SR Majewski, RP Schiavon… - The Astronomical …, 2017 - iopscience.iop.org
Abstract The Apache Point Observatory Galactic Evolution Experiment (APOGEE), one of the
programs in the Sloan Digital Sky Survey III (SDSS-III), has now completed its systematic …

Fundamental parameters and spectral energy distributions of young and field age objects with masses spanning the stellar to planetary regime

JC Filippazzo, EL Rice, J Faherty, KL Cruz… - The Astrophysical …, 2015 - iopscience.iop.org
We combine optical, near-infrared, and mid-infrared spectra and photometry to construct
expanded spectral energy distributions for 145 field age (> 500 Myr) and 53 young (lower …

The CARMENES search for exoplanets around M dwarfs-Stellar atmospheric parameters of target stars with STEPARSYN

E Marfil, HM Tabernero, D Montes… - Astronomy & …, 2021 - aanda.org
We determined effective temperatures, surface gravities, and metallicities for a sample of
343 M dwarfs observed with CARMENES, the double-channel, high-resolution spectrograph …

Angular differential imaging: a powerful high-contrast imaging technique

C Marois, D Lafreniere, R Doyon… - The Astrophysical …, 2006 - iopscience.iop.org
Angular differential imaging is a high-contrast imaging technique that reduces quasistatic
speckle noise and facilitates the detection of nearby companions. A sequence of images is …

Disequilibrium carbon, oxygen, and nitrogen chemistry in the atmospheres of HD 189733b and HD 209458b

JI Moses, C Visscher, JJ Fortney… - The Astrophysical …, 2011 - iopscience.iop.org
We have developed a one-dimensional photochemical and thermochemical kinetics and
diffusion model to study the effects of disequilibrium chemistry on the atmospheric …