activity
20022026
most citedA simple model for the evolution of the dust population in protoplanetary disks

864 citations · 8k across the 144 of their papers we have counts for

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Showing 2014Show all

5 papers · 1 filter

astro-ph.GA2014★ 25 cited

Primordial mass segregation in simulations of star formation?

Richard J. Parker, James E. Dale, Barbara Ercolano

We take the end result of smoothed particle hydrodynamics (SPH) simulations of star formation which include feedback from photoionisation and stellar winds and evolve them for a fu…

astro-ph.SR2014★ 140 cited

The timing and location of dust formation in the remnant of SN 1987A

R. Wesson, M. J. Barlow, M. Matsuura +1

The discovery with the {\it Herschel Space Observatory} of bright far infrared and submm emission from the ejecta of the core collapse supernova SN\,1987A has been interpreted as i…

astro-ph.SR2014★ 168 cited

On the gas content of transitional disks: a VLT/X-Shooter study of accretion and winds

C. F. Manara, L. Testi, A. Natta +4

Transitional disks (TDs) are thought to be a late evolutionary stage of protoplanetary disks with dust depleted inner regions. The mechanism responsible for this depletion is still…

astro-ph.EP2014★ 83 cited

Protoplanetary disc evolution affected by star-disc interactions in young stellar clusters

Giovanni P. Rosotti, James E. Dale, Maria de Juan Ovelar +4

Most stars form in a clustered environment. Therefore, it is important to assess how this environment influences the evolution of protoplanetary discs around young stars. In turn,…

astro-ph.SR2014★ 20 cited

Observations and three-dimensional photoionization modelling of the Wolf-Rayet planetary nebula Abell 48

A. Danehkar, H. Todt, B. Ercolano +1

Recent observations reveal that the central star of the planetary nebula Abell 48 exhibits spectral features similar to massive nitrogen-sequence Wolf-Rayet stars. This raises a pe…