Search Publications

A Wide-Field Hubble Space Telescope Study of the Cluster Cl 0024+1654 at z=0.4. II. The Cluster Mass Distribution
DOI: 10.1086/378633 Bibcode: 2003ApJ...598..804K

Smith, Graham P.; Treu, Tommaso; Smail, Ian +6 more

We present a comprehensive lensing analysis of the rich cluster Cl 0024+1654 (z=0.395) based on panoramic sparse-sampled imaging conducted with the WFPC2 and STIS cameras on board the Hubble Space Telescope. By comparing higher fidelity signals in the limited STIS data with the wider field data available from WFPC2, we demonstrate an ability to de…

2003 The Astrophysical Journal
eHST 225
A Uniform Database of 2.4-45.4 Micron Spectra from the Infrared Space Observatory Short Wavelength Spectrometer
DOI: 10.1086/375443 Bibcode: 2003ApJS..147..379S

Sloan, G. C.; Kraemer, Kathleen E.; Price, Stephan D. +1 more

We present a complete set of all valid SWS full-scan 2.4-45.4 µm spectra processed and renormalized in as uniform a manner as possible. The processing produces a single spectrum for each observation from the 288 individual spectral segments, which are the most processed form available from the ISO archive. The spectra, and the programs used …

2003 The Astrophysical Journal Supplement Series
ISO 225
Dynamical and Physical Properties of a Post-Coronal Mass Ejection Current Sheet
DOI: 10.1086/376982 Bibcode: 2003ApJ...594.1068K

Lin, Jun; Raymond, John C.; Li, Jing +3 more

In the eruptive process of the Kopp-Pneuman type, the closed magnetic field is stretched by the eruption so much that it is usually believed to be ``open'' to infinity. Formation of the current sheet in such a configuration makes it possible for the energy in the coronal magnetic field to quickly convert into thermal and kinetic energies and cause…

2003 The Astrophysical Journal
SOHO 224
Distances to nearby galaxies in Sculptor
DOI: 10.1051/0004-6361:20030170 Bibcode: 2003A&A...404...93K

Sarajedini, A.; Dolphin, A. E.; Grebel, E. K. +7 more

We present an analysis of Hubble Space Telescope/WFPC2 images of nine nearby galaxies in Sculptor. We derive their distances from the luminosity of the tip of the red giant branch stars with a typical accuracy of ~ 12%. Their distances are 4.21 Mpc (Sc 22), 4.92 Mpc (DDO 226), 3.94 Mpc (NGC 253), 3.40 Mpc (KDG 2), 3.34 Mpc (DDO 6), 3.42 Mpc (ESO 5…

2003 Astronomy and Astrophysics
eHST 223
Steps toward interstellar silicate mineralogy. VII. Spectral properties and crystallization behaviour of magnesium silicates produced by the sol-gel method
DOI: 10.1051/0004-6361:20030916 Bibcode: 2003A&A...408..193J

Mutschke, H.; Henning, Th.; Posch, Th. +2 more

Amorphous silicate particles are generally assumed to be the main dust component in the envelopes of oxygen-rich evolved stars and may be considered the precursors of the pure crystalline enstatite and forsterite particles detected by ISO. We present optical constants in the broad wavelength range 0.2-500 mu m for a unique series of pure amorphous…

2003 Astronomy and Astrophysics
ISO 222
Active longitudes in sunspot activity: Century scale persistence
DOI: 10.1051/0004-6361:20030748 Bibcode: 2003A&A...405.1121B

Usoskin, I. G.; Berdyugina, S. V.

A novel analysis of sunspot group data for the past 120 years reveals that sunspots in both northern and southern hemispheres are formed preferably in two persistent active longitudes separated by 180°. In the Carrington reference frame, the active longitudes continuously migrate in phase with respect to the Carrington meridian with a variable rat…

2003 Astronomy and Astrophysics
SOHO 216
An energetic stellar outburst accompanied by circumstellar light echoes
DOI: 10.1038/nature01508 Bibcode: 2003Natur.422..405B

Munari, U.; Sparks, William B.; Bond, Howard E. +6 more

Some classes of stars, including novae and supernovae, undergo explosive outbursts that eject stellar material into space. In 2002, the previously unknown variable star V838 Monocerotis brightened suddenly by a factor of ~104. Unlike a supernova or nova, it did not explosively eject its outer layers; rather, it simply expanded to become…

2003 Nature
eHST 216
A Young White Dwarf Companion to Pulsar B1620-26: Evidence for Early Planet Formation
DOI: 10.1126/science.1086326 Bibcode: 2003Sci...301..193S

Richer, Harvey B.; Hansen, Brad M.; Stairs, Ingrid H. +2 more

The pulsar B1620-26 has two companions, one of stellar mass and one of planetary mass. We detected the stellar companion with the use of Hubble Space Telescope observations. The color and magnitude of the stellar companion indicate that it is an undermassive white dwarf (0.34 +/- 0.04 solar mass) of age 480 × 106 +/- 140 × 106

2003 Science
eHST 214
Direct Detection of a Coronal Mass Ejection-Associated Shock in Large Angle and Spectrometric Coronagraph Experiment White-Light Images
DOI: 10.1086/379098 Bibcode: 2003ApJ...598.1392V

Wu, S. T.; Howard, R. A.; Vourlidas, A. +2 more

The Large Angle and Spectrometric Coronagraph Experiment (LASCO) C2 and C3 coronagraphs recorded a unique coronal mass ejection (CME) on 1999 April 2. The event did not have the typical three-part CME structure and involved a small-filament eruption without any visible overlying streamer ejecta. The event exhibited an unusually clear signature of …

2003 The Astrophysical Journal
SOHO 212
The Structure and Dynamics of Luminous and Dark Matter in the Early-Type Lens Galaxy of 0047-281 at z = 0.485
DOI: 10.1086/345423 Bibcode: 2003ApJ...583..606K

Treu, Tommaso; Koopmans, Léon V. E.

We have measured the kinematic profile of the early-type (E/S0) lens galaxy in the system 0047-281 (z=0.485) with the Echelle Spectrograph and Imager (ESI) on the W. M. Keck II Telescope, as part of the Lenses Structure and Dynamics (LSD) Survey. The central velocity dispersion is σ=229+/-15 km s-1, and the dispersion profile is nearly …

2003 The Astrophysical Journal
eHST 211