Pulsars, transients and relativistic astrophysics

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The emission distribution in SS433

International Conference Recent Advances in Natural Language Processing, RANLP (2006)

Authors:

L Schmidtobreick, K Blundell

Abstract:

We present the results from a large observing campaign where we obtained 61 medium resolution spectra spread over three months. We thus cover roughly five orbits and about half a precession phase. In this paper we describe the analysis of the so-called "stationary" emission lines, which we use to compute Doppler-maps of the emission distribution in the SS433-system. The radial velocities of the individual line components have been analysed. Periodic variations with the orbital period are confirmed, but also variations on longer timescales are found. These long-term variation might be either either related to the precession phase or to some transient phenomen.
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Active galactic nuclei as scaled-up Galactic black holes

Nature Springer Nature 444:7120 (2006) 730-732

Authors:

IM McHardy, E Koerding, C Knigge, P Uttley, RP Fender
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Determining the nature of the faint X-ray source population near the Galactic Centre

(2006)

Authors:

Reba M Bandyopadhyay, Andrew J Gosling, Katherine M Blundell, Philipp Podsiadlowski, Stephen E Eikenberry, Valerie J Mikles, James CA Miller-Jones, Franz E Bauer
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Simultaneous radio/X-ray observations of Cir X-1

(2006)

Authors:

V Tudose, P Soleri, RP Fender, PG Jonker, M van der Klis, AK Tzioumis, RE Spencer
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Jet-dominated advective systems of all mass scales

(2006)

Authors:

Elmar Koerding, Rob Fender
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