237 citations · 1.4k across the 50 of their papers we have counts for
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astro-ph.SR2010
From Bipolar to Elliptical: Morphological Changes in the Temporal Evolution of PN
Martin Huarte Espinosa, Adam Frank, Bruce Balick +4
Proto-planetary nebulae (pPN) and planetary nebulae (PN) seem to be formed by interacting winds from asymptotic giant branch (AGB) stars. The observational issue that most pPN are…
astro-ph.SR2010★ 2 cited
Quantifying the Imprecision of Accretion Theory and Implications for Multi-Epoch Observations of Protoplanetary Discs
Eric G. Blackman, Farrukh Nauman, Richard G. Edgar
If accretion disc emission results from turbulent dissipation, then axisymmetric accretion theory must be used as a mean field theory: turbulent flows are at most axisymmetric only…