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O VI, N V, and C IV in the Galactic Halo. II. Velocity-Resolved Observations with the Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer
DOI: 10.1086/383465 Bibcode: 2004ApJ...607..309I

Shull, J. Michael; Indebetouw, Rémy

We present a survey of N V and O VI (and, where available, C IV) in the Galactic halo, using data from the Far Ultraviolet Spectroscopic Explorer (FUSE) and the Hubble Space Telescope (HST) along 34 sight lines. These ions are usually produced in nonequilibrium processes such as shocks, evaporative interfaces, or rapidly cooling gas, and thus trac…

2004 The Astrophysical Journal
eHST 38
Motion and orientation of magnetic field dips and peaks in the terrestrial magnetosheath
DOI: 10.1029/2003JA010237 Bibcode: 2004JGRA..109.9209H

Balogh, A.; Dandouras, I.; RèMe, H. +2 more

Using data from the four Cluster spacecraft, estimates of the motion of isolated magnetic field dips and peaks in the magnetosheath are presented. Their motion and orientation are deduced using four-spacecraft timing, with typical spacecraft separations of ∼100 km. A set of 39 clear isolated dips and 12 peaks, spread over 4 days, is considered. Th…

2004 Journal of Geophysical Research (Space Physics)
Cluster 37
XMM-Newton Observations of A133: A Weak Shock Passing through the Cool Core
DOI: 10.1086/424807 Bibcode: 2004ApJ...616..157F

Sarazin, Craig L.; Reiprich, Thomas H.; Ehle, M. +5 more

We use XMM-Newton observations of the cluster of galaxies A133 to study the X-ray spectrum of the intracluster medium (ICM). We find a cold front to the southeast of the cluster core. From the pressure profile near the cold front, we derive an upper limit to the velocity of the core relative to the rest of the cluster of less than 230 km s-1<…

2004 The Astrophysical Journal
XMM-Newton 37
A Comparison of the Outer Atmosphere of the ``Flat Activity'' Star τ Ceti (G8 V) with the Sun (G2 V) and α Centauri A (G2 V)
DOI: 10.1086/421044 Bibcode: 2004ApJ...609..392J

Ayres, Thomas R.; Judge, Philip G.; Carlsson, Mats +1 more

Driven by the desire to understand the roles of acoustic and magnetic mechanisms in heating the outer atmospheres of Sun-like stars, we compare solar UV spectra with archival STIS spectra from the Hubble Space Telescope of α Cen A (G2 V) and new STIS spectra of the extremely inactive dwarf star τ Cet (G8 V, V=3.5). The activity of τ Cet shows occa…

2004 The Astrophysical Journal
IUE SOHO eHST 37
In-flight calibration of the Cassini-Radio and Plasma Wave Science (RPWS) antenna system for direction-finding and polarization measurements
DOI: 10.1029/2003JA010261 Bibcode: 2004JGRA..109.9S17V

Gurnett, Donald A.; Fischer, Georg; Lecacheux, Alain +10 more

One major objective of the Cassini mission is the analysis of Saturnian radio emissions of magnetospheric (auroral) as well as atmospheric (lightning) origin. The Radio and Plasma Wave Science (RPWS) experiment is designed to measure the full polarization and the wave vector of the incoming radio waves, allowing us to retrieve information on sourc…

2004 Journal of Geophysical Research (Space Physics)
Cassini 37
Discovery of a Soft Spectral Component and Transient 22.7 Second Quasi-periodic Oscillations of SAX J2103.5+4545
DOI: 10.1086/424825 Bibcode: 2004ApJ...616..463I

Baykal, A.; İnam, S. Ç.; Swank, J. +1 more

XMM-Newton observed SAX J2103.5+4545 on 2003 January 6, while the Rossi X-Ray Timing Explorer (RXTE) was also monitoring the source. Using the RXTE Proportional Counter Array data set between 2002 December 3 and 2003 January 29, the spin period and average spin-up rate during the XMM-Newton observations were found to be 354.7940+/-0.0008 s and (7.…

2004 The Astrophysical Journal
XMM-Newton 37
XMM-Newton observation of the most X-ray-luminous galaxy cluster RX J1347.5-1145
DOI: 10.1051/0004-6361:200400086 Bibcode: 2004A&A...427L...9G

Schindler, S.; Gitti, M.

We report on an XMM-Newton observation of RX J1347.5-1145 (z=0.451), the most luminous X-ray cluster of galaxies currently known, with a luminosity LX = 6.0 ± 0.1 × 1045 erg/s in the [2-10] keV energy band. We present the first temperature map of this cluster, which shows a complex structure. It identifies the cool core and a…

2004 Astronomy and Astrophysics
XMM-Newton 37
Observations of Cold Dust in Nearby Elliptical Galaxies
DOI: 10.1086/422795 Bibcode: 2004ApJ...612..837L

Kuno, Nario; Haas, Martin; Sansom, Anne E. +2 more

Spectral energy distribution (SED) analyses that include new millimeter to far-infrared (FIR) observations obtained with continuum instruments on the Nobeyama and James Clerk Maxwell Telescopes and the Infrared Space Observatory are presented for seven nearby (<45 Mpc) FIR-bright elliptical galaxies. These are analyzed together with archival FI…

2004 The Astrophysical Journal
ISO 37
Infrared Surface Brightness Fluctuations of Magellanic Star Clusters
DOI: 10.1086/421968 Bibcode: 2004ApJ...611..270G

Liu, Michael C.; Bruzual A., Gustavo; González, Rosa A.

We present surface brightness fluctuations (SBFs) in the near-IR for 191 Magellanic star clusters available in the Second Incremental and All Sky Data releases of the Two Micron All Sky Survey (2MASS) and compare them with SBFs of Fornax Cluster galaxies and with predictions from stellar population models as well. We also construct color-magnitude…

2004 The Astrophysical Journal
eHST 37
Bimodal distribution of the autocorrelation function in gamma-ray bursts
DOI: 10.1051/0004-6361:20034567 Bibcode: 2004A&A...418..487B

Borgonovo, L.

Autocorrelation functions (ACFs) are studied for a sample of 16 long gamma-ray bursts (GRBs) with known redshift z, that were observed by the BATSE and Konus experiments. When corrected for cosmic time dilation, the ACF shows a bimodal distribution. A narrow width class (11 bursts) has at half-maximum a mean width τ'0=1.6 s with a relat…

2004 Astronomy and Astrophysics
INTEGRAL 37