activity
20092023
most citedDiscovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager

559 citations · 6.7k across the 108 of their papers we have counts for

collaborators
Showing 2021Show all

11 papers · 1 filter

astro-ph.IM2021★ 5 cited

UV Spectropolarimetry with Polstar: Protoplanetary Disks

John P. Wisniewski, Andrei V. Berdyugin, Svetlana V. Berdyugina +13

Polstar is a proposed NASA MIDEX mission that would feature a high resolution UV spectropolarimeter capable of measure all four Stokes parameters onboard a 60cm telescope. The miss…

astro-ph.EP2021★ 7 cited

CI Tau: A controlled experiment in disk-planet interaction

Dhruv Muley, Ruobing Dong

CI Tau is a young (~2 Myr) T Tauri system with a substantial near-infrared excess in its SED, indicating that the protoplanetary disk extends very close to its star. This is seemin…

astro-ph.EP2021★ 27 cited

GW Ori: circumtriple rings and planets

Jeremy L. Smallwood, Rebecca Nealon, Cheng Chen +4

GW Ori is a hierarchical triple star system with a misaligned circumtriple protoplanetary disc. Recent ALMA observations have identified three dust rings with a prominent gap at $1…

astro-ph.EP2021★ 19 cited

Keck/OSIRIS Pa high-contrast imaging and updated constraints on PDS~70b

Taichi Uyama, Chen Xie, Yuhiko Aoyama +11

We present a high-contrast imaging search for Pa line emission from protoplanets in the PDS~70 system with Keck/OSIRIS integral field spectroscopy. We applied the high-resolutio…

astro-ph.EP2021★ 25 cited

Investigating Protoplanetary Disk Cooling through Kinematics: Analytical GI Wiggle

Cristiano Longarini, Giuseppe Lodato, Claudia Toci +4

It is likely that young protostellar disks undergo a self-gravitating phase. Such systems are characterized by the presence of a spiral pattern that can be either in a quasi-steady…

astro-ph.SR2021★ 37 cited

Massive compact disks around FU Orionis-type young eruptive stars revealed by ALMA

Á. Kóspál, F. Cruz-Sáenz de Miera, J. A. White +14

FU Orionis-type objects (FUors) are low-mass pre-main sequence stars undergoing a temporary, but significant increase of mass accretion rate from the circumstellar disk onto the pr…