activity
20182022
most citedNested Dust Shells around the Wolf-Rayet Binary WR 140 observed with JWST

60 citations · 167 across the 8 of their papers we have counts for

collaborators

11 papers

astro-ph.SR202221 cited

Radiation-driven acceleration in the expanding WR140 dust shell

Yinuo Han, Peter G. Tuthill, Ryan M. Lau +1

The Wolf-Rayet (WR) binary system WR140 is a close (0.9-16.7 mas) binary star consisting of an O5 primary and WC7 companion and is known as the archetype of episodic dust-producing…

astro-ph.SR202260 cited

Nested Dust Shells around the Wolf-Rayet Binary WR 140 observed with JWST

Ryan M. Lau, Matthew J. Hankins, Yinuo Han +29

Massive colliding-wind binaries that host a Wolf-Rayet (WR) star present a potentially important source of dust and chemical enrichment in the interstellar medium (ISM). However, t…

astro-ph.SR20228 cited

Smoke on the wind: dust nucleation in archetype colliding wind pinwheel WR104

A. Soulain, A. Lamberts, F. Millour +2

A handful of binary Wolf-Rayet stars are known to harbour spectacular spiral structures spanning a few hundred AU. These systems host some of the highest dust production rates in t…

astro-ph.EP2022

Two Rings and a Marginally Resolved, 5 AU, Disk Around LkCa 15 Identified Via Near Infrared Sparse Aperture Masking Interferometry

Dori Blakely, Logan Francis, Doug Johnstone +10

Sparse aperture masking interferometry (SAM) is a high resolution observing technique that allows for imaging at and beyond a telescope's diffraction limit. The technique is ideal…

astro-ph.IM202221 cited

The James Webb Space Telescope Aperture Masking Interferometer

A. Soulain, A. Sivaramakrishnan, P. Tuthill +10

In less than a year, the James Webb Space Telescope (JWST) will inherit the mantle of being the world's pre-eminent infrared observatory. JWST will carry with it an Aperture Maskin…

astro-ph.EP202112 cited

First MATISSE L-band observations of HD 179218. Is the inner 10 au region rich in carbon dust particles?

E. Kokoulina, A. Matter, B. Lopez +58

Carbon is one of the most abundant components in the Universe. While silicates have been the main focus of solid phase studies in protoplanetary discs (PPDs), little is known about…