activity
19952022
most citedCompetitive accretion in embedded stellar cluster

606 citations · 8.8k across the 72 of their papers we have counts for

collaborators

69 papers

astro-ph.EP2022★ 7 cited

Stellar winds can affect gas dynamics in debris disks and create observable belt winds

Quentin Kral, James Pringle, Luca Matrà +1

Context: Gas is now detected in many extrasolar systems around mature stars aged between 10 Myr to 1 Gyr with planetesimal belts. Gas in these mature disks is thought to be…

astro-ph.EP2021★ 16 cited

A molecular wind blows out of the Kuiper belt

Quentin Kral, J. E. Pringle, Aurélie Guilbert-Lepoutre +9

Gas has been detected in many exoplanetary systems (10 Myr), thought to be released in the destruction of volatile-rich planetesimals orbiting in exo-Kuiper belts. In this lette…

astro-ph.HE2020★ 21 cited

Accretion discs with non-zero central torque

C. J. Nixon, J. E. Pringle

We present analytical and numerical solutions for accretion discs subject to a non-zero central torque. We express this in terms of a single parameter, , which is the ratio of o…

astro-ph.SR2020★ 13 cited

Emission from elliptical streams of dusty debris around white dwarfs

C. J. Nixon, J. E. Pringle, E. R. Coughlin +2

White dwarfs are routinely observed to have polluted atmospheres, and sometimes significant infrared excesses, that indicate ongoing accretion of circumstellar dust and rocky debri…

astro-ph.SR2020★ 9 cited

Polarization measurements of the polluted white dwarf G29-38

Daniel V. Cotton, Jeremy Bailey, J. E. Pringle +3

We have made high precision polarimetric observations of the polluted white dwarf G29-38 with the HIgh Precision Polarimetric Instrument 2. The observations were made at two differ…

astro-ph.HE2020★ 7 cited

Strong surface outflows on accretion discs

C. J. Nixon, J. E. Pringle

In order to provide an explanation for the unexpected radial brightness distribution of the steady accretion discs seen in nova-like variables, Nixon & Pringle (2019) proposed that…