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Origins of the Highly Ionized Gas along the Line of Sight toward HD 116852
Richter, Philipp; Sembach, Kenneth R.; Savage, Blair D. +5 more
We present Hubble Space Telescope Imaging Spectrograph (HST/STIS) and Far Ultraviolet Spectroscopic Explorer (FUSE) observations of high ion interstellar ultraviolet absorption along the sight line to HD 116852. At a distance of 4.8 kpc, HD 116852 is an O9 III star lying in the low Galactic halo, -1.3 kpc from the plane of the Galaxy in the direct…
Density and Temperature Measurements in a Solar Active Region
Winebarger, Amy R.; Warren, Harry P.
We present electron density and temperature measurements from an active region observed above the limb with the Solar Ultraviolet Measurements of Emitted Radiation spectrometer on the Solar and Heliospheric Observatory. Density-sensitive line ratios from Si VIII and S X indicate densities greater than 108 cm-3 as high as 200"…
Dust in Hot Gas: Far-Infrared Emission from Three Local Elliptical Galaxies
Brighenti, Fabrizio; Mathews, William G.; Bregman, Jesse D. +1 more
We present far-IR Infrared Space Observatory observations of three early-type galaxies in the Virgo Cluster. The data were recorded using the ISOPHOT instrument in both the P32 oversampled maps and the P39/37 sparse maps. The maps reach the limiting sensitivity of the ISOPHOT instrument at 60, 90, and 180 µm. Two of the most prominent ellipt…
Dynamics of the Lyα and C IV Emitting Gas in 3C 273
Paltani, Stéphane; Türler, Marc
In this paper we study the variability properties of the Lyα and C IV emission lines in 3C 273 using archival International Ultraviolet Explorer observations. Our data show for the first time the existence of variability on timescales of several years. We study the spatial distribution and the velocity field of the emitting gas by performing detai…
Stellar Motions in the Polar Ring Galaxy NGC 4650A
Swaters, Rob A.; Rubin, Vera C.
We present the first measurement of the stellar kinematics in the polar ring of NGC 4650A. There is well-defined rotation, with the stars and gas rotating in the same direction, and with similar amplitude. The gaseous and stellar kinematics suggest an approximately flat rotation curve, providing further support for the hypothesis that the polar ma…
GRB 030227 : The first multiwavelength afterglow of an INTEGRAL GRB
Pian, E.; Palazzi, E.; Greiner, J. +39 more
We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (
Maximum Entropy imaging with INTEGRAL/SPI data
Strong, A. W.
The application of the Maximum Entropy method for sky imaging with the SPI instrument on INTEGRAL is described. While intended primarily for extended emission, point sources are also mapped by this method. The technique is implemented as the program spiskymax in the data analysis distribution provided by the INTEGRAL Science Data Centre. We briefl…
Impact of aerosols present in Titan's atmosphere on the CASSINI radar experiment
Rodriguez, S.; Encrenaz, P.; Dobrijevic, M. +4 more
Simulations of Titan's atmospheric transmission and surface reflectivity have been developed in order to estimate how Titan's atmosphere and surface properties could affect performances of the Cassini radar experiment. In this paper we present a selection of models for Titan's haze, vertical rain distribution, and surface composition implemented i…
Multisite observations of the PMS delta Scuti star V351 Ori
Ripepi, V.; Palla, F.; Marconi, M. +12 more
We present the results of multisite observations spanning two years on the pre-main-sequence (PMS) star V351 Ori. A total of around 180 hours of observations over 29 nights have been collected, allowing us to measure five different periodicities, most likely related to the delta Scuti variability of V351 Ori. Comparison with the predictions of lin…
Near-Infrared Observations of BL Lacertae Host Galaxies
Giavalisco, Mauro; Cheung, C. C.; Urry, C. Megan +1 more
Multiband near-infrared images of 12 BL Lacertae objects were obtained with the 2.5 m telescope at the Las Campanas Observatory in order to determine the properties of their underlying host galaxies. Resolved emission was clearly detected in eight of the lowest redshift targets (up to z~0.3) and was modeled with a de Vaucouleurs r1/4 su…