Benchmark ages for the Gaia benchmark stars
CL Sahlholdt, S Feltzing, L Lindegren… - Monthly Notices of the …, 2019 - academic.oup.com
In the era of large-scale surveys of stars in the Milky Way, stellar ages are crucial for
studying the evolution of the Galaxy. But determining ages of field stars is notoriously …
studying the evolution of the Galaxy. But determining ages of field stars is notoriously …
The mean longitudinal magnetic field and its uses in radial-velocity surveys
F Rescigno, A Mortier, X Dumusque… - Monthly Notices of …, 2024 - academic.oup.com
This work focuses on the analysis of the mean longitudinal magnetic field as a stellar activity
tracer in the context of small exoplanet detection and characterization in radial-velocity (RV) …
tracer in the context of small exoplanet detection and characterization in radial-velocity (RV) …
MOVES–I. The evolving magnetic field of the planet-hosting star HD189733
HD189733 is an active K dwarf that is, with its transiting hot Jupiter, among the most studied
exoplanetary systems. In this first paper of the Multiwavelength Observations of an …
exoplanetary systems. In this first paper of the Multiwavelength Observations of an …
Magnetized winds and their influence in the escaping upper atmosphere of HD 209458b
C Villarreal D'Angelo, A Esquivel… - Monthly Notices of …, 2018 - academic.oup.com
Lyman α observations during an exoplanet transit have proved to be very useful to study the
interaction between the stellar wind and the planetary atmosphere. They have been …
interaction between the stellar wind and the planetary atmosphere. They have been …
Characterization of the HD 219134 multiplanet system I. Observations of stellar magnetism, wind, and high-energy flux
CP Folsom, L Fossati, BE Wood… - Monthly Notices of …, 2018 - academic.oup.com
ABSTRACT HD 219134 hosts several planets, with seven candidates reported, and the two
shortest period planets are rocky (4–5 M⊕) and transit the star. Here, we present …
shortest period planets are rocky (4–5 M⊕) and transit the star. Here, we present …
Spectroscopic binaries in the Solar Twin Planet Search program: from substellar–mass to M dwarf companions
Previous studies on the rotation of Sun-like stars revealed that the rotational rates of young
stars converge towards a well-defined evolution that follows a power-law decay. It seems …
stars converge towards a well-defined evolution that follows a power-law decay. It seems …
Probing the magnetic fields of starspots with transit mapping
Context. Starspots, regions of strong magnetic fields, serve as indicators of stellar activity
and the dynamo mechanism at play in the interior of stars. The magnetic fields of main …
and the dynamo mechanism at play in the interior of stars. The magnetic fields of main …
Models of star-planet magnetic interaction
A Strugarek - arXiv preprint arXiv:1704.03254, 2017 - arxiv.org
Magnetic interactions between a planet and its environment are known to lead to
phenomena such as aurorae and shocks in the solar system. The large number of close-in …
phenomena such as aurorae and shocks in the solar system. The large number of close-in …
Signatures of star-planet interactions
EL Shkolnik, J Llama - arXiv preprint arXiv:1712.02814, 2017 - arxiv.org
Planets interact with their host stars through gravity, radiation and magnetic fields, and for
those giant planets that orbit their stars within $\sim $10 stellar radii ($\sim $0.1 AU for a sun …
those giant planets that orbit their stars within $\sim $10 stellar radii ($\sim $0.1 AU for a sun …
Exploring the robustness of Keplerian signals to the removal of active and telluric features
We examine the influence of activity-and telluric-induced radial velocity (RV) signals on high-
resolution spectra taken with an iodine absorption cell. We exclude 2-spectral chunks …
resolution spectra taken with an iodine absorption cell. We exclude 2-spectral chunks …