[HTML][HTML] Binary stars in the new millennium

X Chen, Z Liu, Z Han - Progress in Particle and Nuclear Physics, 2024 - Elsevier
Binary stars are as common as single stars. Binary stars are of immense importance to
astrophysicists because that they allow us to determine the masses of the stars independent …

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 …

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 …

The Star–Planet Composition Connection

JK Teske - Annual Review of Astronomy and Astrophysics, 2024 - annualreviews.org
The mantra “know thy star, know thy planet” has proven to be very important for many
aspects of exoplanet science. Here I review how stellar abundances inform our …

Constraints on the Spindown of Fully Convective M Dwarfs Using Wide Field Binaries

EK Pass, D Charbonneau, JM Irwin… - The Astrophysical …, 2022 - iopscience.iop.org
M dwarfs remain active over longer timescales than their Sunlike counterparts, with
potentially devastating implications for the atmospheres of their planets. However, the age at …

CARMENES: high-resolution spectra and precise radial velocities in the red and infrared

A Quirrenbach, PJ Amado, I Ribas… - Ground-based and …, 2018 - spiedigitallibrary.org
The design and construction of CARMENES has been presented at previous SPIE
conferences. It is a next-generation radial-velocity instrument at the 3.5 m telescope of the …

Sub-m s−1 upper limits from a deep HARPS-N radial-velocity search for planets orbiting HD 166620 and HD 144579

A Anna John, A Collier Cameron… - Monthly Notices of …, 2023 - academic.oup.com
Minimizing the impact of stellar variability in radial velocity (RV) measurements is a critical
challenge in achieving the 10 cm s− 1 precision needed to hunt for Earth twins. Since 2012 …

The TIME Table: rotation and ages of cool exoplanet host stars

E Gaidos, Z Claytor, R Dungee, A Ali… - Monthly Notices of the …, 2023 - academic.oup.com
Age is a stellar parameter that is both fundamental and difficult to determine. Among middle-
aged M dwarfs, the most prolific hosts of close-in and detectable exoplanets, gyrochronology …

PENELLOPE: The ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES)-I. Survey presentation and accretion properties …

CF Manara, A Frasca, L Venuti, M Siwak… - Astronomy & …, 2021 - aanda.org
The evolution of young stars and disks is driven by the interplay of several processes,
notably the accretion and ejection of material. These processes, critical to correctly describe …

Identical or fraternal twins? The chemical homogeneity of wide binaries from Gaia DR2

K Hawkins, M Lucey, YS Ting, A Ji… - Monthly Notices of …, 2020 - academic.oup.com
One of the high-level goals of Galactic archaeology is chemical tagging of stars across the
Milky Way to piece together its assembly history. For this to work, stars born together must be …