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20022026
most citedA Catalog of Quasar Properties from SDSS DR7

1.5k citations

Showing astro-ph.EPShow all

27 papers · 1 filter

astro-ph.EP20263 cited

Exploring the conditions for forming planetesimals by the streaming instability and planetary systems by pebble accretion

Anders Johansen, Wladimir Lyra

The streaming instability and pebble accretion are two physical mechanisms with demonstrated potentials to drive, respectively, the formation of planetesimals and the growth of pla…

astro-ph.EP20261 cited

A distant brown dwarf coplanar to a warm Jupiter and a hot super-Earth

Matías I. Jones, Luca Naponiello, Trifon Trifonov +21

In transiting planetary systems, in which planetary sizes are accurately determined from transit observations, the presence of transit-timing variations (TTVs), especially when com…

astro-ph.EP2026

Excitation and Damping of Oscillation Modes in Gaseous Planets

Jim Fuller, Marzia Parisi, Steve Markham +2

The excitation and damping mechanisms for oscillation modes of gas giant planets are undetermined. We show that differential rotation may greatly enhance convective viscosity in gi…

astro-ph.EP2025

New Orbital Constraints for YSES 1 b and HR 2562 B from High-Precision Astrometry and Planetary Radial Velocities

Jonathan Roberts, William Thompson, Jason J. Wang +20

We present new VLTI/GRAVITY astrometry and updated orbit fits for the directly imaged companions YSES 1 b and HR 2562 B, substellar objects straddling the planet-brown dwarf bounda…

astro-ph.EP20239 cited

Are NH and CO ice present on Miranda?

Riley A. DeColibus, Nancy J. Chanover, Richard J. Cartwright

Published near-infrared spectra of the four largest classical Uranian satellites display the presence of discrete deposits of CO ice, along with subtle absorption features arou…

astro-ph.EP202377 cited

Direct imaging discovery of a super-Jovian around the young Sun-like star AF Leporis

Robert J. De Rosa, Eric L. Nielsen, Zahed Wahhaj +5

(abridged) Expanding the sample of directly imaged companions to nearby, young stars that are amenable to detailed astrometric and spectroscopic studies is critical for the continu…