activity
20032018
most citedDynamical aspects of isoscaling

44 citations · 326 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.GA2018★ 6 cited

The Owl and other strigiform nebulae: multipolar cavities within a filled shell

Ma. T. García-Díaz, W. Steffen, W. J. Henney +4

We present the results of long-slit echelle spectroscopy and deep narrow-band imaging of the Owl Nebula (NGC 3587), obtained at the \textit{Observatorio Astronómico Nacional, San P…

astro-ph.CO2016★ 21 cited

Fine-structure constant constraints on dark energy: II. Extending the parameter space

C. J. A. P. Martins, A. M. M. Pinho, P. Carreira +3

Astrophysical tests of the stability of fundamental couplings, such as the fine-structure constant , are a powerful probe of new physics. Recently these measurements, combined w…

astro-ph.SR2015★ 23 cited

Evidence for a [WR] or WEL-type binary nucleus in the bipolar planetary nebula Vy 1-2

S. Akras, P. Boumis, J. Meaburn +3

We present high-dispersion spectroscopic data of the compact planetary nebula Vy 1-2, where high expansion velocities up to 100 km/s are found in the Ha, [N II] and [O III] emissio…

astro-ph.SR2014★ 7 cited

The Present and Future of Planetary Nebula Research. A White Paper by the IAU Planetary Nebula Working Group

K. B. Kwitter, R. H. Méndez, M. Peña +10

We present a summary of current research on planetary nebulae and their central stars, and related subjects such as atomic processes in ionized nebulae, AGB and post-AGB evolution.…

astro-ph.SR2013★ 31 cited

Two rings but no fellowship: LoTr 1 and its relation to planetary nebulae possessing barium central stars

A. A. Tyndall, D. Jones, H. M. J. Boffin +7

LoTr 1 is a planetary nebula thought to contain an intermediate-period binary central star system (that is, a system with an orbital period, P, between 100 and, say, 1500 days). Th…

nucl-th2012★ 2 cited

Coulomb forces in neutron star crusts

C. O. Dorso, P. A. Giménez Molinelli, J. A. López +1

We study the role the proton-electron gas interaction has on the formation of nuclear structures in neutron star crusts. Using a classical molecular dynamics model we study isospin…