activity
20092026
most citedStellar obliquities in exoplanetary systems

187 citations · 711 across the 25 of their papers we have counts for

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Showing 2022Show all

8 papers · 1 filter

astro-ph.EP2022★ 9 cited

Radial velocity confirmation of a hot super-Neptune discovered by TESS with a warm Saturn-mass companion

E. Knudstrup, D. Gandolfi, G. Nowak +59

We report the discovery and confirmation of the planetary system TOI-1288. This late G dwarf harbours two planets: TOI-1288 b and TOI-1288 c. We combine TESS space-borne and ground…

astro-ph.EP2022★ 72 cited

TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain

Fei Dai, Kento Masuda, Corey Beard +60

Convergent disk migration has long been suspected to be responsible for forming planetary systems with a chain of mean-motion resonances (MMR). Dynamical evolution over time could…

astro-ph.IM2022★ 6 cited

CHARA/SPICA: a 6-telescope visible instrument for the CHARA Array

Denis Mourard, Philippe Berio, Cyril Pannetier +25

With a possible angular resolution down to 0.1-0.2 millisecond of arc using the 330 m baselines and the access to the 600-900 nm spectral domain, the CHARA Array is ideally configu…

astro-ph.EP2022★ 27 cited

A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system

Luisa Maria Serrano, Davide Gandolfi, Alexander J. Mustill +47

It is commonly accepted that exoplanets with orbital periods shorter than 1 day, also known as ultra-short period (USP) planets, formed further out within their natal protoplanetar…

astro-ph.EP2022★ 20 cited

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

Quang H. Tran, Brendan P. Bowler, Michael Endl +38

We report the discovery of two transiting planets around the bright ( mag) main sequence F7 star TOI-1670 by the Transiting Exoplanet Survey Satellite. TOI-1670 b is a sub-N…

astro-ph.EP2022★ 23 cited

A Radial Velocity Study of the Planetary System of Pi Mensae: Improved Planet Parameters for PI Mensae c and a Third Planet on a 125-d Orbit

Artie P. Hatzes, Davide Gandolfi, Judith Korth +33

Pi Men hosts a transiting planet detected by the TESS space mission and an outer planet in a 5.7-yr orbit discovered by RV surveys. We studied this system using new radial velocity…

astro-ph.EP2022★ 187 cited

Stellar obliquities in exoplanetary systems

Simon H. Albrecht, Rebekah I. Dawson, Joshua N. Winn

The rotation of a star and the revolutions of its planets are not necessarily aligned. This article reviews the measurement techniques, key findings, and theoretical interpretation…

astro-ph.SR2022★ 9 cited

DI Herculis Revisited: Starspots, Gravity Darkening, and 3-D Obliquities

Yan Liang, Joshua N. Winn, Simon H. Albrecht

DI Herculis is an eclipsing binary famous for a longstanding disagreement between theory and observation of the apsidal precession rate, which was resolved when both stars were fou…