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Persistent North-South Alignment of the Solar Supergranulation
Toomre, Juri; Lisle, Jason P.; Rast, Mark P.
We have found evidence of an alignment of the solar supergranulation in the direction parallel to the Sun's rotation axis. Signatures of the alignment are apparent in both time-averaged images and in three-dimensional power spectra. The north-south organization is persistent in time, extending over many supergranular lifetimes. It occurs over a wi…
Solar cycle dependence of the helium focusing cone from SOHO/UVCS observations. Electron impact rates and associated pickup ions
Bertaux, J. -L.; Raymond, J. C.; Uzzo, M. +5 more
The Ultraviolet Coronograph on board SOHO (UVCS) has observed the 58.4 nm glow of the interplanetary He focusing cone at regular intervals since 1996. The intensity decrease with time already observed during the first two years (Michels et al. \cite{michels}) has dramatically amplified during the solar activity increase. Intensities seem to reach …
The Unusual Tidal Dwarf Candidate in the Merger System NGC 3227/3226: Star Formation in a Tidal Shock?
Forbes, Duncan A.; Schinnerer, Eva; Mundell, Carole G. +2 more
We report the discovery of active star formation in the H I cloud associated with the interacting Seyfert system NGC 3227/3226 that was originally identified as a candidate tidal dwarf galaxy (TDG) by Mundell et al. and that we name J1023+1952. We present broadband optical B, R, I (from the Isaac Newton Telescope), and ultraviolet images (from XMM…
Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study
Lundin, R.; Balogh, A.; Dandouras, I. +14 more
Available from http://www.copernicus.org/site/EGU/annales/22/7/2325.htm?FrameEngine=false;
On the Wolf-Rayet counterpart to IC 10 X-1
Crowther, P. A.; Clark, J. S.
Recent CHANDRA observations of the starburst galaxy
Studies of Microflares in RHESSI Hard X-Ray, Big Bear Solar Observatory Hα, and Michelson Doppler Imager Magnetograms
Krucker, Säm; Liu, Chang; Qiu, Jiong +2 more
In this paper, we present a study of the morphology of 12 microflares jointly observed by RHESSI in the energy range from 3 to 15 keV and by Big Bear Solar Observatory (BBSO) at the Hα line. They are A2-B3 events in GOES classification. From their time profiles, we find that all of these microflares are seen in soft X-ray, hard X-ray, and Hα wavel…
Long-lived triaxiality in the dynamically old elliptical galaxy NGC 4365: a limit on chaos and black hole mass
Bacon, Roland; Emsellem, Eric; Peletier, Reynier F. +1 more
Supermassive black holes in the centres of giant elliptical galaxies are thought to be capable of inducing chaos and eliminating or preventing triaxiality in their hosts if they are sufficiently massive. We address whether this process operates in real systems, by modelling the stellar kinematics of the old elliptical NGC 4365. This galaxy has a m…
Spectral evolution of weak bursts from SGR 1806-20 observed with INTEGRAL
Hurley, K.; Götz, D.; Mereghetti, S. +1 more
We report on bursts from the Soft Gamma-Ray Repeater SGR 1806-20 detected with INTEGRAL in October 2003, during a period of moderate activity of the source. The spectral and temporal properties of 21 short bursts are consistent with those found in previous observations, even if these bursts are among the faintest observed in the 15-200 keV range f…
A Period and a Prediction for the Of?p Spectrum Alternator HD 191612
Corcoran, Michael F.; Walborn, Nolan R.; Bond, Howard E. +7 more
The observational picture of the enigmatic O-type spectrum variable HD 191612 has been sharpened substantially. A symmetrical, low-amplitude light curve with a period near 540 days has recently been reported from Hipparcos photometry. This period satisfies all of the spectroscopy since at least 1982, including extensive new observations during 200…
Hubble Space Telescope NICMOS Variability Study of Massive Stars in the Young Dense Galactic Starburst NGC 3603
Bergeron, E.; Moffat, A. F. J.; Marchenko, S. V. +4 more
We have used the relatively long data string of the 1997-1999 NICMOS focus tests on NGC 3603 to extract ~J-band light curves for several hundred stars in the cluster core. Given the relatively modest photometric precision [σ(J)>=0.05 mag], we were able to isolate only a half-dozen variable candidates with peak-to-valley amplitudes above ~0.2 ma…