The orientation between a star's spin axis and a planet's orbital plane provides valuable
information about the system's formation and dynamical history. For non-transiting planets at …

Context. Emission lines that are indicative of active accretion have been observed for a
number of low-mass companions (M< 30 M Jup) to stars. Line variability is ubiquitous on …

We report a new evaluation of the accretion properties of PDS 70b obtained with the Very
Large Telescope/Multi Unit Spectroscopic Explorer. The main difference from the previous …

Accretion signatures from bound brown dwarf and protoplanetary companions provide
evidence for ongoing planet formation, and accreting substellar objects have enabled new …

Accreting protoplanets are windows into planet formation processes, and high-contrast
differential imaging is an effective way to identify them. We report results from the Giant …

The Comprehensive Archive of Substellar and Planetary Accretion Rates - IOPscience This
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …

In the core-accretion formation scenario of gas giants, most of the gas accreting onto a
planet is processed through an accretion shock. In this series of papers we study this shock …

GQ Lup B is a forming brown dwarf companion (M∼ 10–30 MJ) showing evidence for an
infrared excess associated with a disk surrounding the companion itself. Here we present …

Giant planets grow by accreting gas through circumplanetary disks, but little is known about
the timescale and mechanisms involved in the planet-assembly process because few …

Context. Several detections of wide-orbit planet-mass/substellar companions around young
solar-like stars were reported in the last decade. The origin of those possible planets is still …