Search Publications

On the Interaction between Convection and Magnetic Fields
DOI: 10.1086/374313 Bibcode: 2003ApJ...588.1183C

Cattaneo, Fausto; Emonet, Thierry; Weiss, Nigel

Turbulent convection in the solar photosphere can act as a small-scale dynamo, maintaining a disordered magnetic field that is locally intense. On the other hand, convection is inhibited in the presence of a strong, externally imposed magnetic field, as for instance, in a sunspot. Large-scale, three-dimensional, numerical experiments on highly non…

2003 The Astrophysical Journal
SOHO 227
Determination of the gas-to-dust ratio in nearby dense clouds using X-ray absorption measurements
DOI: 10.1051/0004-6361:20030942 Bibcode: 2003A&A...408..581V

Grosso, N.; Montmerle, T.; Feigelson, E. D. +3 more

We present a comparison of the gas and dust properties of the dense interstellar matter in six nearby star-forming regions (d<500 pc): rho Oph, Cha I, R CrA, IC 348, NGC 1333, and Orion. We measure from Chandra and XMM-Newton observations the X-ray absorption toward pre-main sequence stars (PMS) without accretion disks (i.e., Class III sources)…

2003 Astronomy and Astrophysics
XMM-Newton 227
Current sheet structure near magnetic X-line observed by Cluster
DOI: 10.1029/2002GL016730 Bibcode: 2003GeoRL..30.1579R

Balogh, A.; Zhang, T. L.; Klecker, B. +9 more

During the interval 0947-0951 UT on 1 October 2001, when Cluster was located at X GSM = -16.4 R E near Z GSM = 0 in the pre-midnight magnetotail, the Cluster barycenter crosses the neutral sheet four times. High speed proton flow, with reversal from tailward to Earthward, was detected during the crossings. Us…

2003 Geophysical Research Letters
Cluster 226
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