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20182026
most citedA Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS

95 citations · 591 across the 37 of their papers we have counts for

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Showing 2023Show all

8 papers · 1 filter

astro-ph.GA2023

K2 results for "young" -rich stars in the Galaxy

V. Grisoni, C. Chiappini, A. Miglio +11

The origin of apparently young -rich stars in the Galaxy is still a matter of debate in Galactic archaeology, whether they are genuinely young or might be products of binary evo…

astro-ph.GA2023★ 34 cited

Cluster Ages to Reconstruct the Milky Way Assembly (CARMA) I. The final word on the origin of NGC6388 and NGC6441

Davide Massari, Fernando Aguado-Agelet, Matteo Monelli +11

We present CARMA, the Cluster Ages to Reconstruct the Milky Way Assembly project, that aims at determining precise and accurate age measurements for the entire system of known Gala…

astro-ph.SR2023★ 17 cited

An asteroseismic age estimate of the open cluster NGC 6866 using Kepler and Gaia

K. Brogaard, T. Arentoft, A. Miglio +10

Asteroseismology of solar-like oscillations in giant stars allow the derivation of their masses and radii. For members of open clusters this allows an age estimate of the cluster w…

astro-ph.SR2023★ 19 cited

Asteroseismology and Spectropolarimetry of the Exoplanet Host Star Serpentis

Travis S. Metcalfe, Derek Buzasi, Daniel Huber +31

The bright star Ser hosts a hot Neptune with a minimum mass of 13.6 and a 15.5 day orbit. It also appears to be a solar analog, with a mean rotation period of 25.8 d…

astro-ph.SR2023★ 23 cited

A close-in giant planet escapes engulfment by its star

Marc Hon, Daniel Huber, Nicholas Z. Rui +39

When main-sequence stars expand into red giants, they are expected to engulf close-in planets. Until now, the absence of planets with short orbital periods around post-expansion, c…

astro-ph.GA2023★ 14 cited

A Unified Exploration of the Chronology of the Galaxy

Amalie Stokholm, Víctor Aguirre Børsen-Koch, Dennis Stello +2

The Milky Way has distinct structural stellar components linked to its formation and subsequent evolution, but disentangling them is nontrivial. With the recent availability of hig…

astro-ph.SR2023

Did Kepler-444 have a long-lived convective core?

Mark Lykke Winther, Víctor Aguirre Børsen-Koch, Jakob Lysgaard Rørsted +2

With the greater power to infer the state of stellar interiors provided by asteroseismology, it has become possible to study the survival of initially convective cores within stars…

astro-ph.GA2023★ 13 cited

Time evolution of Ce as traced by APOGEE using giant stars observed with the Kepler, TESS and K2 missions

G. Casali, V. Grisoni, A. Miglio +11

Abundances of s-capture process elements in stars with exquisite asteroseismic, spectroscopic, and astrometric constraints offer a novel opportunity to study stellar evolution, nuc…