Search Publications

Candidates of z ~= 5.5-7 Galaxies in the Hubble Space Telescope Ultra Deep Field
DOI: 10.1086/424690 Bibcode: 2004ApJ...612L..93Y

Yan, Haojing; Windhorst, Rogier A.

We report results from our z~=5.5-7 galaxy search in the Hubble Space Telescope Ultra Deep Field (UDF). Using the 400 orbit of Advanced Camera for Surveys data, we found 108 plausible 5.5<=z<=6.5 (or z~=6 for short) candidates to mAB(z850)=30.0 mag. The contamination to the sample, due to either image artifacts or known…

2004 The Astrophysical Journal
eHST 145
Hubble Space Telescope STIS Ultraviolet Spectral Evidence of Outflow in Extreme Narrow-Line Seyfert 1 Galaxies. II. Modeling and Interpretation
DOI: 10.1086/422089 Bibcode: 2004ApJ...611..125L

Leighly, Karen M.

We present modeling to explore the conditions of the broad-line-emitting gas in two extreme narrow-line Seyfert 1 galaxies, using the observational results described in the first paper of this series. Photoionization modeling using CLOUDY was conducted for the broad blueshifted wind lines and the narrow, symmetric, rest-wavelength-centered disk li…

2004 The Astrophysical Journal
eHST 144
A Numerical Study of the Breakout Model for Coronal Mass Ejection Initiation
DOI: 10.1086/423887 Bibcode: 2004ApJ...614.1028M

Antiochos, S. K.; Phillips, A.; MacNeice, P. +3 more

A leading theory for the initiation of coronal mass ejections (CMEs) is the breakout model, in which magnetic reconnection above a filament channel is responsible for disrupting the coronal magnetic field. We present the first simulations of the complete breakout process including the initiation, the plasmoid formation and ejection, and the eventu…

2004 The Astrophysical Journal
SOHO 144
Surprising Sun: A New Step Towards a Complete Picture?
DOI: 10.1103/PhysRevLett.93.211102 Bibcode: 2004PhRvL..93u1102T

García, R. A.; Turck-Chièze, S.; Piau, L. +5 more

Important revisions of the solar model ingredients have appeared recently. We first show that the updated CNO composition suppresses the anomalous position of the Sun in the known galactic enrichment. The following law, He/H=0.075+44.6 O/H in number fraction, is now compatible with all the indicators. We then suggest some directions of investigati…

2004 Physical Review Letters
SOHO 144
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