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20152026
most citedA Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS

95 citations · 642 across the 24 of their papers we have counts for

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Showing 2023Show all

5 papers · 1 filter

astro-ph.SR2023★ 2 cited

Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems -- A census of oscillating red-giants and main-sequence stars in Gaia DR3 binaries

P. G. Beck, D. H. Grossmann, L. Steinwender +23

Binary systems constitute a valuable astrophysics tool for testing our understanding of stellar structure and evolution. Systems containing a oscillating component are interesting…

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.SR2023★ 5 cited

Solar-like oscillations in Cephei A as seen through SONG and TESS

E. Knudstrup, M. N. Lund, M. Fredslund Andersen +11

Fundamental stellar parameters such as mass and radius are some of the most important building blocks in astronomy, both when it comes to understanding the star itself and when der…

astro-ph.SR2023★ 1 cited

Spectroscopic identification of rapidly rotating red giant stars in APOKASC-3 and APOGEE DR16

Rachel A. Patton, Marc H. Pinsonneault, Lyra Cao +6

Rapidly rotating red giant stars are astrophysically interesting but rare. In this paper we present a catalog of 3217 active red giant candidates in the APOGEE DR16 survey. We use…

astro-ph.SR2023★ 16 cited

Red Horizontal Branch stars: an asteroseismic perspective

Massimiliano Matteuzzi, Josefina Montalbán, Andrea Miglio +7

Robust age estimates of red giant stars are now possible thanks to the precise inference of their mass based on asteroseismic constraints. However, there are cases where such age e…