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Evidence for Strong and Weak Turbulence Processes in the Source Region of a Local Type III Radio Burst
MacDowall, R. J.; Thejappa, G.
We present the Ulysses Unified Radio and Plasma Wave Experiment (URAP) observations of a local type III radio burst and the associated plasma wave activity generated in the vicinity of the spacecraft. These observations represent the first clear evidence of (1) the occurrence of ion-acoustic waves as well as whistlers in close association with Lan…
The Hubble Deep Field and the disappearing dwarf galaxies
Ferguson, Henry C.; Babul, Arif
Several independent lines of reasoning, both theoretical and observational, suggest that the very faint (B>~24) galaxies seen in deep images of the sky are small low-mass galaxies that have experienced a short epoch of star formation at redshifts 0.5<~z<~1 and have since faded into low-luminosity, low-surface-brightness objects. Such a sc…
Dissecting Capella's Corona: GHRS Spectra of the Fe XXI λ1354 and He II λ1640 Lines from Each of the Capella Stars
Brown, Alexander; Wood, Brian E.; Osten, Rachel A. +1 more
We report on moderate (λ/Δλ = 20,000) and high (λ/Δλ = 90,000) resolution spectra of the 104-day period Capella binary system (HD 34029) obtained with Hubble Space Telescope's Goddard High-Resolution Spectrometer (GHRS) on 1995 September 9 and 1996 April 9. The observations include a long-duration, moderate-resolution spectrum of the coronal Fe XX…
Radiative Transfer Models of Emission and Absorption in the H2O 6 Micron Vibration-Rotation Band toward Orion-BN-KL
Cernicharo, José; van Dishoeck, Ewine F.; Wright, Christopher M. +2 more
We report the spectrum of Orion-BN/KL between 5.3 and 7.2 µm observed with the Short Wavelength Spectrometer (SWS) on board the Infrared Space Observatory. H2O lines of the ν2=1-0 bending mode with λ < 6.3 µm (the R-branch) are observed in absorption, while lines with λ > 6.3 µm (the P-branch) are obse…
Halo stars in the immediate solar neighbourhood
Jahreiß, H.; Fuchs, B.
We have searched the Fourth Catalogue of Nearby Stars for halo stars and identified 15 subdwarfs and a high velocity white dwarf in the solar neighbourhood. This search was motivated mainly by the recent determinations of MACHO masses of about 0.5cal M_sun, which are typical for halo dwarfs. The local mass density of these stars is 1.5*10(-4) cal …
Bar-driven evolution of S0s: the edge-on galaxy NGC 4570
van den Bosch, Frank C.; Emsellem, Eric
We present circumstantial evidence that the central region of the edge-on S0 galaxy NGC 4570, which harbours a 150-pc scale nuclear disc in addition to its main outer disc, has been shaped under the influence of a small (~500 pc) bar. This is based on the discovery of two edge-on rings, the locations of which are consistent with the inner Lindblad…
A New Analysis of RR Lyrae Kinematics in the Solar Neighborhood
Martin, John C.; Morrison, Heather L.
Full space velocities are computed for a sample of 130 nearby RR Lyrae variables using both ground-based and Hipparcos proper motions. In many cases proper motions for the same star from multiple sources have been averaged to produce approximately a factor of 2 improvement in the transverse space velocity errors. In most cases, this exceeds the ac…
Clouds of High Contrast on Uranus
Karkoschka, Erich
Cosmological Parameters from Multiple-Arc Gravitational Lensing Systems. I. Smooth Lensing Potentials
Link, Robert; Pierce, Michael J.
We describe a new approach for the determination of cosmological parameters using gravitational lensing systems with multiple arcs. We exploit the fact that a given cluster can produce multiple arcs from sources over a broad range in redshift. The coupling between the critical radius of a single arc and the projected mass density of the lensing cl…
Seismic Holography of Solar Activity
Braun, D. C.; Lindsey, C.; Fan, Y. +1 more
Helioseismic images of sunspots show a remarkable acoustic anomaly surrounding the sunspot. We applied the computational formalism of ``helioseismic holography'' to SOHO-MDI observations to render acoustic images of NOAA AR 7973, an active region containing a moderately large sunspot. The results of this study are based on simple ``acoustic power …