activity
20142026
most citedOn the X-ray temperature of hot gas in diffuse nebulae

37 citations · 131 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Photoionization modelling of circumstellar nebulae using irregular grains

P. Jiménez-Hernández, S. J. Arthur, D. Guirado +4

We study the effects of using the optical properties of irregular hexahedral grains in photoionization models of circumstellar nebulae around evolved stars. Dust opacities for the…

astro-ph.SR2026

Formation and X-ray emission from hot bubbles in planetary nebulae - III. The impact of [Wolf-Rayet]-type winds

Rogelio Orozco-Duarte, Jesús A. Toalá, S. Jane Arthur +3

We use radiation-hydrodynamical simulations to investigate the formation and synthetic X-ray emission of hot bubbles within planetary nebulae (PNe) driven by the powerful winds of…

astro-ph.GA2018★ 37 cited

On the X-ray temperature of hot gas in diffuse nebulae

J. A. Toalá, S. J. Arthur

X-ray emitting diffuse nebulae around hot stars are observed to have soft-band temperatures in the narrow range [1-3] K, independent of the stellar wind parameters an…

astro-ph.GA2016★ 31 cited

Turbulence in the Ionized Gas of the Orion Nebula

S. J. Arthur, S. -N. X. Medina, W. J. Henney

In order to study the nature, origin, and impact of turbulent velocity fluctuations in the ionized gas of the Orion Nebula, we apply a variety of statistical techniques to observed…

astro-ph.SR2014★ 30 cited

Expansion of hydrogen-poor knots in the born-again planetary nebulae A30 and A78

Xuan Fang, Martin A. Guerrero, Ramon A. Marquez-Lugo +8

We analyze the expansion of hydrogen-poor knots and filaments in the born-again planetary nebulae A30 and A78 based on Hubble Space Telescope (HST) images obtained almost 20 yr apa…

astro-ph.GA2014★ 33 cited

Turbulence in simulated HII regions

S. -N. X. Medina, S. J. Arthur, W. J. Henney +2

We investigate the scale dependence of fluctuations inside a realistic model of an evolving turbulent HII region and to what extent these may be studied observationally. We find th…