activity
20032026
most citedX-ray irradiated protoplanetary disk atmospheres I: Predicted emission line spectrum and photoevaporation

188 citations · 1.5k across the 42 of their papers we have counts for

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Showing 2007Show all

7 papers · 1 filter

astro-ph200764 cited

The hydrogen-deficient knot of the `born again' planetary nebula Abell 58 (V605 Aql)

R. Wesson, M. J. Barlow, X-W. Liu +3

We have analysed deep optical spectra of the `born-again' planetary nebula Abell 58 and its hydrogen-deficient knot, surrounding V605 Aql, which underwent a nova-like eruption in 1…

astro-ph2007125 cited

X-ray enabled MOCASSIN: a 3D code for photoionized media

Barbara Ercolano, Peter R. Young, Jeremy J. Drake +1

We present a new version of the fully 3D photoionization and dust radiative transfer code, MOCASSIN, that uses a Monte Carlo approach for the transfer of radiation. The X-ray enabl…

astro-ph200733 cited

X-ray Fluorescent Fe Kalpha Lines from Stellar Photospheres

Jeremy J. Drake, Barbara Ercolano, Douglas A. Swartz

X-ray spectra from stellar coronae are reprocessed by the underlying photosphere through scattering and photoionization events. While reprocessed X-ray spectra reaching a distant o…

astro-ph20079 cited

The Detectability of Neon Fluorescence and Measurement of the Solar Photospheric Neon Abundance

Jeremy J. Drake, Barbara Ercolano

Monte Carlo calculations of the Ne K line fluoresced by coronal x-rays and emitted near the temperature minimum region of the solar atmosphere have been employed to investigate…

astro-ph2007100 cited

Hierarchical Star-Formation in M33: Fundamental properties of the star-forming regions

N. Bastian, B. Ercolano, M. Gieles +4

Star-formation within galaxies appears on multiple scales, from spiral structure, to OB associations, to individual star clusters, and often sub-structure within these clusters. Th…

astro-ph200743 cited

The effects of spatially distributed ionisation sources on the temperature structure of HII region

B. Ercolano, N. Bastian, G. Stasinska

Spatially resolved studies of star forming regions show that the assumption of spherical geometry is not realistic in most cases, with a major complication posed by the gas being i…