activity
19992023
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 3.3k across the 82 of their papers we have counts for

collaborators

83 papers

astro-ph.SR2023

Eta Carinae: the dissipating occulter is an extended structure

Theodore R. Gull, Henrik Hartman, Mairan Teodoro +10

Previous STIS long-slit observations of Eta Carinae identified numerous absorption features in both the stellar spectrum, and in the adjacent nebular spectra, along our line-of-sig…

astro-ph.HE2023★ 9 cited

Delayed Development of Cool Plasmas in X-ray Flares from kappa1 Ceti

Kenji Hamaguchi, Jeffrey W. Reep, Vladimir Airapetian +3

The Neutron star Interior Composition ExploreR (NICER) X-ray observatory observed two powerful X-ray flares equivalent to superflares from the nearby young solar-like star, kappa1…

astro-ph.SR2022★ 60 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.HE2022★ 7 cited

NICER X-ray Observations of Eta Carinae During its Most Recent Periastron Passage

David Espinoza-Galeas, Michael Francis Corcoran, Kenji Hamaguchi +12

We report high-precision X-ray monitoring observations in the 0.4-10 keV band of the luminous, long-period colliding-wind binary Eta Carinae up to and through its most recent X-ray…

astro-ph.SR2022

Eta Carinae: an evolving view of the central binary, its interacting winds and its foreground ejecta

Theodore R. Gull, D. John Hillier, Henrik Hartman +13

FUV spectra of Eta Car, recorded across two decades with HST/STIS, document multiple changes in resonant lines caused by dissipating extinction in our line of sight. The FUV flux h…

astro-ph.HE2021★ 18 cited

Competitive X-ray and Optical Cooling in the Collisionless Shocks of WR 140

A. M. T. Pollock, M. F. Corcoran, I. R. Stevens +9

WR 140 is a long-period, highly eccentric Wolf-Rayet star binary system with exceptionally well-determined orbital and stellar parameters. Bright, variable X-ray emission is genera…