activity
19952008
most citedNeutral H density at the termination shock: a consolidation of recent results

58 citations · 234 across the 27 of their papers we have counts for

collaborators

48 papers

astro-ph200858 cited

Neutral H density at the termination shock: a consolidation of recent results

M. Bzowski, E. Moebius, S. Tarnopolski +2

We discuss a consolidation of determinations of the density of neutral interstellar H at the nose of the termination shock carried out with the use of various data sets, techniques…

astro-ph2008

Searching for white dwarfs candidates in Sloan Digital Sky Survey Data

Mirosław Należyty, Agnieszka Majczyna, Anna Ciechanowska +1

Large amount of observational spectroscopic data are recently available from different observational projects, like Sloan Digital Sky Survey. It's become more urgent to identify wh…

cond-mat.dis-nn200817 cited

Spin Waves in the Ferromagnetic Ground State of the Kagome Staircase System Co3V2O8

M. Ramazanoglu, C. P. Adams, J. P. Clancy +6

Inelastic neutron scattering measurements were performed on single crystal Co3V2O8 wherein magnetic cobalt ions reside on distinct spine and cross-tie sites within kagome staircase…

astro-ph2008

Monte Carlo Simulations of Star Clusters - IV. Calibration of the Monte Carlo Code and Comparison with Observations for the Open Cluster M67

Mirek Giersz, Douglas C. Heggie, Jarrod R. Hurley

We outline the steps needed in order to incorporate the evolution of single and binary stars into a particular Monte Carlo code for the dynamical evolution of a star cluster. We ca…

astro-ph20071 cited

Hot Jupiters and Central Cavities of Protoplanetary Discs

Szymon Starczewski, Artur J. Gawryszczak, Richard Wunsch +1

We investigate numerically the orbital evolution of massive extrasolar planets within central cavities of their parent protoplanetary discs. Assuming that they arrive at the inner…

astro-ph2007

Monte Carlo simulations of star clusters with primordial binaries. Comparison with N-body simulations and observations

Mirek Giersz, Douglas C. Heggie

We outline the steps needed in to calibrate the Monte Carlo code in order to perform large scale simulations of real globular clusters. We calibrate the results against -body si…