activity
20002023
most citedBalmer-Dominated Spectra of Nonradiative Shocks in the Cygnus Loop, RCW 86 and Tycho Supernova Remnants

206 citations · 1.9k across the 38 of their papers we have counts for

collaborators
Showing 2022Show all

6 papers · 1 filter

astro-ph.HE2022★ 1 cited

Morphology of Shocked Lateral Outflows in Colliding Hydrodynamic Flows

R. N. Markwick, A. Frank, J. Carroll-Nellenback +6

Supersonic interacting flows occurring in phenomena such as protostellar jets give rise to strong shocks, and have been demonstrated in several laboratory experiments. To study suc…

astro-ph.GA2022★ 4 cited

Length-scales and Dynamics of Carina's Western Wall

Turlough Downes, Patrick Hartigan, Andrea Isella

We present a variety of analyses of the turbulent dynamics of the boundary of a photo-dissociation region (PDR) in the Carina Nebula using high resolution ALMA observations. Using…

astro-ph.GA2022★ 3 cited

ALMA Datacubes and Continuum Maps of the Irradiated Western Wall in Carina

Patrick Hartigan, Maxwell Hummel, Andrea Isella +1

We present ALMA observations of the continuum and line emission of CO, CO, CO, and [C I] for a portion of the G287.38-0.62 (Car 1-E) region in the Carina star-…

physics.plasm-ph2022★ 14 cited

Perpendicular subcritical shock structure in a collisional plasma experiment

D. R. Russell, G. C. Burdiak, J. J. Carroll-Nellenback +13

We present a study of perpendicular subcritical shocks in a collisional laboratory plasma. Shocks are produced by placing obstacles into the super-magnetosonic outflow from an inve…

astro-ph.GA2022★ 88 cited

PDRs4All: A JWST Early Release Science Program on radiative feedback from massive stars

Olivier Berné, Émilie Habart, Els Peeters +134

Massive stars disrupt their natal molecular cloud material through radiative and mechanical feedback processes. These processes have profound effects on the evolution of interstell…

physics.plasm-ph2022★ 11 cited

Experimental observations of detached bow shock formation in the interaction of a laser-produced plasma with a magnetized obstacle

Joseph M. Levesque, Andy S. Liao, Patrick Hartigan +14

The magnetic field produced by planets with active dynamos, like the Earth, can exert sufficient pressure to oppose supersonic stellar wind plasmas, leading to the formation of a s…