Pulsars, transients and relativistic astrophysics

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Fluid dynamics - Spinning discs in the lab

NATURE 444:7117 (2006) 281-+
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On the Binary Nature of SS 433

Chapter in Close Binaries in the 21st Century: New Opportunities and Challenges, Springer Nature (2006) 269-272

Authors:

Linda Schmidtobreick, Katherine Blundell
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On the binary nature of SS 433

ASTROPHYSICS AND SPACE SCIENCE 304:1-4 (2006) 271-274

Authors:

Linda Schmidtobreick, Katherine Blundell
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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

Authors:

MA Urbaneja, A Herrero, R-P Kudritzki, F Najarro, SJ Smartt, J Puls, DJ Lennon, LJ Corral
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Astrophysics and space science: From X-ray binaries to quasars: Black holes on all mass scales

, 2005

Authors:

TJ MacCarone, RP Fender, LC Ho

Abstract:

This volume brings together contributions from many of the world's leading authorities on black hole accretion. The papers within represent part of a new movement to make use of the relative advantages of studying stellar mass and supermassive black holes, and to bring together the knowledge gained from the two approaches. The topics discussed include observational and theoretical work-variability, spectroscopy, disk-jet connections, and multi-wavelength campaigns on black holes. © Springer 2005. All Rights Reserved.
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