activity
19952001
most citedDiscovery of Correlated Behavior Between the HXR and the Radio Bands in Cygnus X-3

85 citations · 254 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2001

Far-Infrared ISO Limits on Dust Disks around Millisecond Pulsars

T. J. W. Lazio, J. Fischer, R. S. Foster

We report 60 and 90 micron observations of 7 millisecond pulsars with the ISOPHOT instrument and describe our analysis procedures. No pulsars were detected, and typical (3σ) upper…

astro-ph2001★ 58 cited

A Dual Frequency, Multi-Year Monitoring Program of Compact Radio Sources

T. Joseph W. Lazio, E. B. Waltman, F. D. Ghigo +3

We present light curves for 149 sources monitored with the Green Bank Interferometer. The light curves are at two radio frequencies (approximately 2.5 and 8.2 GHz) and range from 3…

astro-ph1998★ 85 cited

Discovery of Correlated Behavior Between the HXR and the Radio Bands in Cygnus X-3

M. L. McCollough, C. R. Robinson, S. N. Zhang +8

Using CGRO/BATSE hard X-ray (HXR) data and GHz radio monitoring data from the Green Bank Interferometer (GBI), we have performed a long term study ( 1800 days) of the unusual…

astro-ph1997★ 42 cited

Long-Term Flux Monitoring of LSI +61 303 at 2.25 and 8.3 GHz

P. S. Ray, R. S. Foster, E. B. Waltman +2

LSI +61 303 is an exotic binary system consisting of a ~10 Msun B star and a compact object which is probably a neutron star. The system is associated with the interesting radio so…

astro-ph1997★ 33 cited

Discovery of a non-blazar gamma-ray transient near the Galactic plane: GRO J1838-04

M. Tavani, R. Mukherjee, J. R. Mattox +6

We report the discovery of a remarkable gamma-ray transient source near the Galactic plane, GRO J1838-04. This source was serendipitously discovered by EGRET in June 1995 with a pe…

astro-ph1996★ 34 cited

Cygnus X-3 in outburst : quenched radio emission, radiation losses and variable local opacity

R. P. Fender, S. J. Bell Burnell, E. B. Waltman +3

We present multiwavelength observations of Cygnus X-3 during an extended outburst in 1994 February - March. Intensive radio monitoring at 13.3, 3.6 & 2.0 cm is complemented by obse…