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Signatures of Core-envelope Rotational Misalignment in the Mixed-mode Asteroseismology of Kepler-56
Published 2025-01-01“…Upon applying the revised asteroseismic observational methodology that results from this theoretical discussion to revisit Kepler-56—a red giant with a misaligned planetary system—I find that its core and envelope rotate around different rotational axes. …”
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Spin-down of Solar-mass Protostars in Magnetospheric Accretion Paradigm
Published 2025-01-01“…Stellar spin is one of the fundamental quantities that characterize a star itself and its planetary system. Nevertheless, stellar spin-down mechanisms in protostellar and pre-main-sequence stellar phases have been a long-standing problem in star formation theory. …”
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Doppler cross-correlation spectroscopy as a path to the detection of Earth-like planets
Published 2023-06-01“…In the middle of the 20th century, a paradigm shift appeared concerning the expected frequency of planetary systems in the galaxy ...a shift induced by the observation of the rotational velocities of low main sequence stars (Struve 1952)!…”
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Gaia astrometry and exoplanetary science: DR2, (E)DR3, and beyond
Published 2023-06-01“…I review the recent impact of Gaia astrometry in the exoplanet field, both in terms of characterization of the orbits and masses of planetary systems and the properties of their host stars. …”
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The Deuterium Isotopic Ratio of Water Released From the Martian Caps as Measured With TGO/NOMAD
Published 2022-06-01Get full text
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Exoplanet science with SPIRou: near-infrared precision velocimetry and spectropolarimetry
Published 2023-03-01“…SPIRou, installed at the Canada–France–Hawai’i telescope, was designed to explore such planetary systems and characterize their properties. With a wide spectral range and large resolving power, SPIRou is also optimized for transmission spectroscopy and for investigating the chemical composition of exoplanetary atmospheres.…”
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Demographics of M Dwarf Binary Exoplanet Hosts Discovered by TESS
Published 2025-01-01“…However, 20%–30% of M dwarfs have companions that can impact the formation and evolution of planetary systems. We use high-resolution imaging and Gaia astrometry to detect stellar companions around M dwarf exoplanet hosts discovered by TESS and determine the projected separation and estimated stellar masses for each system. …”
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Dynamics of Small, Constant-size Particles in a Protoplanetary Disk with an Embedded Protoplanet
Published 2025-01-01“…Hydrodynamical simulations of protoplanetary disk dynamics are useful tools for understanding the formation of planetary systems, including our own. Approximations are necessary to make these simulations computationally tractable. …”
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Imaging exoplanets with coronagraphic instruments
Published 2023-03-01“…Exoplanetary science is a very active field of astronomy nowadays, with questions still opened such as how planetary systems form and evolve (occurrence, process), why such a diversity of exoplanets is observed (mass, radius, orbital parameters, temperature, composition), and what are the interactions between planets, circumstellar disk and their host star. …”
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