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The host galaxies of luminous quasars
DOI: 10.1111/j.1365-2966.2004.08315.x Bibcode: 2004MNRAS.355..196F

Baum, Stefi A.; O'Dea, Christopher P.; Dunlop, James S. +5 more

We present the results of a deep Hubble Space Telescope (HST)/Wide Field and Planetary Camera 2 imaging study of 17 quasars at z~= 0.4, designed to determine the properties of their host galaxies. The sample consists of quasars with absolute magnitudes in the range -24 >=MV>=- 28, allowing us to investigate host galaxy properties …

2004 Monthly Notices of the Royal Astronomical Society
eHST 144
Disk and Halo Wide Binaries from the Revised Luyten Catalog: Probes of Star Formation and MACHO Dark Matter
DOI: 10.1086/380442 Bibcode: 2004ApJ...601..289C

Gould, Andrew; Chanamé, Julio

We present a catalog of 1147 candidate common proper motion binaries selected from the revised New Luyten Two-Tenths Catalog (NLTT). Among these, we identify 999 genuine physical pairs using the measured proper-motion difference and the relative positions of each binary's components on a reduced proper motion (RPM) diagram. The RPM positions also …

2004 The Astrophysical Journal
Hipparcos 144
A multiwavelength study of solar flare waves. II. Perturbation characteristics and physical interpretation
DOI: 10.1051/0004-6361:20034333 Bibcode: 2004A&A...418.1117W

Magdalenić, J.; Vršnak, B.; Hanslmeier, A. +2 more

The study of solar flare waves - globally propagating wave-like disturbances usually observed in Hα as Moreton waves - has recently come back into focus prompted by the observation of coronal waves in the EUV with the SOHO/EIT instrument (``EIT waves"), and in several additional wavelength channels. We study 12 flare wave events in order to determ…

2004 Astronomy and Astrophysics
SOHO 143
An Unveiling Event in the Type 2 Active Galactic Nucleus NGC 4388:A Challenge for a Parsec-Scale Absorber
DOI: 10.1086/424380 Bibcode: 2004ApJ...615L..25E

Fiore, F.; Elvis, Martin; Miller, J. M. +3 more

We present two Rossi X-Ray Timing Explorer (RXTE) Proportional Counter Array (PCA) observations of the type 2 Seyfert galaxy NGC 4388 caught in an unusual low X-ray absorption state. The observations were triggered by a detection in the 1.5-3 keV band of the RXTE all-sky monitor. NGC 4388 was found at a somewhat high continuum level [f(2-10 keV)=8…

2004 The Astrophysical Journal
XMM-Newton 143
Discovery of Face-on Counterparts of Chain Galaxies in the Tadpole Advanced Camera for Surveys Field
DOI: 10.1086/383312 Bibcode: 2004ApJ...604L..21E

Elmegreen, Bruce G.; Elmegreen, Debra Meloy; Hirst, Amelia C.

The background field of the Tadpole galaxy image taken with the Hubble Space Telescope Advanced Camera for Surveys contains 87 clump clusters that are probably low-inclination versions of the 69 chain galaxies that we found in a previous paper. This conclusion follows from the similarity in colors and apparent magnitudes of the brightest clumps in…

2004 The Astrophysical Journal
eHST 140
Radar: The Cassini Titan Radar Mapper
DOI: 10.1007/s11214-004-1438-9 Bibcode: 2004SSRv..115...71E

Lorenz, R. D.; Soderblom, L. A.; Ostro, S. J. +19 more

The Cassini RADAR instrument is a multimode 13.8 GHz multiple-beam sensor that can operate as a synthetic-aperture radar (SAR) imager, altimeter, scatterometer, and radiometer. The principal objective of the RADAR is to map the surface of Titan. This will be done in the imaging, scatterometer, and radiometer modes. The RADAR altimeter data will pr…

2004 Space Science Reviews
Cassini 139
Role of projection effects on solar coronal mass ejection properties: 1. A study of CMEs associated with limb activity
DOI: 10.1029/2003JA010149 Bibcode: 2004JGRA..109.3103B

St. Cyr, O. C.; Stanger, A. L.; Burkepile, J. T. +2 more

Many properties of Coronal Mass Ejections (CMEs), such as size, location and brightness, have been determined from measurements of white light coronal observations. We expect the average properties derived from these measurements contain systematic inaccuracies due to projection effects and suggest that CME properties are most accurately determine…

2004 Journal of Geophysical Research (Space Physics)
SOHO 139
Subgalactic Clumps at High Redshift: A Fragmentation Origin?
DOI: 10.1086/422179 Bibcode: 2004ApJ...611...20I

Gerhard, Ortwin; Westera, Pieter; Immeli, Andreas +1 more

We investigate the origin of the clumpy structures observed at high redshift, such as chain galaxies. We use a three-dimensional chemodynamical simulation describing the dynamics of stars and a two-phase interstellar medium, as well as feedback processes from the stars. For high efficiency of energy dissipation in the cold cloud medium, the initia…

2004 The Astrophysical Journal
eHST 139
Solar magnetic elements at 0.1 arcsec resolution. General appearance and magnetic structure
DOI: 10.1051/0004-6361:20040436 Bibcode: 2004A&A...428..613B

Hansteen, V. H.; Carlsson, M.; Berger, T. E. +6 more

New observations of solar magnetic elements in a remnant active region plage near disk center are presented. The observations were obtained at the recently commissioned Swedish 1-m Solar Telescope on La Palma. We examine a single 430.5 nm G-band filtergram that resolves ∼70 km (0.1 arcsec) structures and find new forms of magnetic structures in th…

2004 Astronomy and Astrophysics
SOHO 138
Discovery of Hard Nonthermal Pulsed X-Ray Emission from the Anomalous X-Ray Pulsar 1E 1841-045
DOI: 10.1086/423129 Bibcode: 2004ApJ...613.1173K

Kuiper, L.; Hermsen, W.; Mendez, M.

We report the discovery of nonthermal pulsed X-ray/soft gamma-ray emission up to ~150 keV from the anomalous 11.8 s X-ray pulsar AXP 1E 1841-045 located near the center of supernova remnant Kes 73 using Rossi X-Ray Timing Explorer (RXTE) Proportional Counter Array and High Energy X-Ray Timing Experiment (HEXTE) data. The morphology of the double-p…

2004 The Astrophysical Journal
INTEGRAL XMM-Newton 137