activity
20032009
most citedVariation of Inner Radius of Dust Torus in NGC4151

69 citations · 135 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.CO200969 cited

Variation of Inner Radius of Dust Torus in NGC4151

Shintaro Koshida, Yuzuru Yoshii, Yukiyasu Kobayashi +8

The long-term optical and near infrared monitoring observations for a type 1 act ive galactic nucleus NGC 4151 were carried out for six years from 2001 to 2006 b y using the MAGNUM…

astro-ph200844 cited

Possibility of Detecting Moons of Pulsar Planets Through Time-of-Arrival Analysis

Karen M. Lewis, Penny D. Sackett, Rosemary A. Mardling

The perturbation caused by planet-moon binarity on the time-of-arrival signal of a pulsar with an orbiting planet is derived for the case in which the orbits of the moon and the pl…

astro-ph200622 cited

Discovery of an X-ray Jet and Extended Jet Structure in the Quasar PKS 1055+201

D. A. Schwartz, H. L. Marshall, J. E. J. Lovell +10

This letter reports rich X-ray jet structures found in the Chandra observation of PKS 1055+201. In addition to an X-ray jet coincident with the radio jet we detect a region of exte…

astro-ph2005

Detection of 75+ pulsation frequencies in the Delta Scuti star FG Vir

M. Breger, P. Lenz, V. Antoci +9

Extensive photometric multisite campaigns of the Delta Scuti variable FG Vir are presented. For the years 2003 and 2004, 926 hours of photometry at the millimag precision level wer…

astro-ph2004

Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared

H. C. Woodruff, M. Eberhardt, T. Driebe +9

We present K-band commissioning observations of the Mira star prototype o Cet obtained at the ESO Very Large Telescope Interferometer (VLTI) with the VINCI instrument and two sider…

astro-ph2004

Modelling the spectral energy distribution of galaxies. III. Attenuation of stellar light in spiral galaxies

Richard. J. Tuffs, Cristina C. Popescu, Heinrich J. Voelk +2

We present new calculations of the attenuation of stellar light from spiral galaxies using geometries for stars and dust which can reproduce the entire spectral energy distribution…