Extended inverse Compton enussion from distant powerful radio galaxies
ESA SP PUBL 604 (2006) 611-612
Abstract:
Chandra observations of 3C432, 3C191 and B2 0902+34 are presented as part of an ongoing search for inverse-Compton scattering of the cosmic microwave background (CMB) from high redshift radio sources (Schwartz, 2000). The energy density of the CMB increases with redshift, z, as (1 + Z)(4), so the relatively high redshift of these powerful radio galaxies makes them good candidates for detecting extended inverse-Compton scattering along the radio jet axis: we do indeed detect radio-aligned X-ray emission.Fluid dynamics - Spinning discs in the lab
NATURE 444:7117 (2006) 281-+
On the Binary Nature of SS 433
Chapter in Close Binaries in the 21st Century: New Opportunities and Challenges, Springer Nature (2006) 269-272
On the binary nature of SS 433
ASTROPHYSICS AND SPACE SCIENCE 304:1-4 (2006) 271-274
Blue Luminous Stars in Nearby Galaxies: Quantitative Spectral Analysis of M33 B-Type Supergiant Stars**The WHT is operated on the island of La Palma by the ING in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. ****Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
The Astrophysical Journal American Astronomical Society 635:1 (2005) 311-335