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88 papers · 1 filter
High speed photometry of faint cataclysmic variables - VI. Car2, V1040 Cen, Ha 075648, IL Nor (Nova Nor 1893), HS Pup (Nova Pup 1963), SDSS J2048-06, CSS 081419-005022 and CSS 112634-100210
Patrick A. Woudt, Brian Warner
We have observed 8 faint cataclysmic variable stars photometrically. The nova-like Car2 was extensively sampled but showed little variability. V1040 Cen was observed near the end o…
Be/X-ray binary SXP6.85 undergoes large Type II outburst in the Small Magellanic Cloud
L. J. Townsend, M. J. Coe, V. A. McBride +6
The Small Magellanic Cloud (SMC) Be/X-ray binary pulsar SXP6.85 = XTE J0103-728 underwent a large Type II outburst beginning on 2008 August 10. The source was consistently seen for…
Time and Spacetime: The Crystallizing Block Universe
George F. R. Ellis, Tony Rothman
The nature of the future is completely different from the nature of the past. When quantum effects are significant, the future shows all the signs of quantum weirdness, including d…
The y-sky: diffuse spectral distortions of the cosmic microwave background
Cyril Pitrou, Francis Bernardeau, Jean-Philippe Uzan
The non-linear evolution of the energy density of the radiation is shown to induce spectral distortions of the cosmic microwave background both at recombination and during the reio…
Very long-term X-ray variations in LMXBs: solar cycle-like variations in the donor?
M. M. Kotze, P. A. Charles
Long-term monitoring of Low Mass X-ray Binaries (LMXBs) by the All Sky Monitor on board the Rossi X-ray Timing Explorer now covers ~13 yrs and shows that certain LMXB types display…
Constraining chameleon field theories using the GammeV afterglow experiments
A. Upadhye, J. H. Steffen, A. Weltman
The GammeV experiment has constrained the couplings of chameleon scalar fields to matter and photons. Here we present a detailed calculation of the chameleon afterglow rate underly…