activity
19982023
most citedChaotic motion and spiral structure in self-consistent models of rotating galaxies

66 citations · 137 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2023

GRBAlpha: the smallest astrophysical space observatory -- Part 1: Detector design, system description and satellite operations

András Pál, Masanori Ohno, László Mészáros +42

Aims. Since launched on 2021 March 22, the 1U-sized CubeSat GRBAlpha operates and collects scientific data on high-energy transients, making it the smallest astrophysical space obs…

astro-ph.GA2016★ 29 cited

The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering

Ben Chehade, T. Shanks, J. Findlay +10

We present a new redshift survey, the 2dF Quasar Dark Energy Survey pilot (2QDESp), which consists of quasars from deg of the southern sky, base…

astro-ph2006★ 66 cited

Chaotic motion and spiral structure in self-consistent models of rotating galaxies

N. Voglis, I. Stavropoulos, C. Kalapotharakos

Dissipationless N-body models of rotating galaxies, iso-energetic to a non-rotating model, are examined as regards the mass in regular and in chaotic motion. The values of their sp…

astro-ph2004★ 42 cited

The K-band intensity profile of R Leonis probed by VLTI/VINCI

D. Fedele, M. Wittkowski, F. Paresce +3

We present near-infrared K-band interferometric measurements of the Mira star R Leonis obtained in April 2001 and January 2002 with the VLTI, the commissioning instrument VINCI, an…

astro-ph1998

RXTE Observations of Cygnus X-1: Broad-Band Spectra and High-Resolution Timing

K. Pottschmidt, J. Wilms, M. A. Nowak +3

We present results from a 20 ksec RXTE observation of the black hole candidate Cyg X-1. We apply self-consistent accretion disk corona models to these hard state data and show that…

astro-ph1998

RXTE Observations of LMC X-1 and LMC X-3

J. Wilms, M. A. Nowak, J. B. Dove +4

Of all known persistent stellar-mass black hole candidates, only LMC X-1 and LMC X-3 consistently show spectra that are dominated by a soft, thermal component. We present results f…