Search Publications

A soft solid surface on Titan as revealed by the Huygens Surface Science Package
DOI: 10.1038/nature04211 Bibcode: 2005Natur.438..792Z

Banaszkiewicz, Marek; Zarnecki, John C.; Lorenz, Ralph D. +23 more

The surface of Saturn's largest satellite-Titan-is largely obscured by an optically thick atmospheric haze, and so its nature has been the subject of considerable speculation and discussion. The Huygens probe entered Titan's atmosphere on 14 January 2005 and descended to the surface using a parachute system. Here we report measurements made just a…

2005 Nature
Huygens 100
Density-potential pairs for spherical stellar systems with Sérsic light profiles and (optional) power-law cores
DOI: 10.1111/j.1365-2966.2005.09269.x Bibcode: 2005MNRAS.362..197T

Graham, Alister W.; Terzić, Balša

Popular models for describing the luminosity-density profiles of dynamically hot stellar systems (e.g. Jaffe, Hernquist, Dehnen) were constructed with the desire to match the deprojected form of an R1/4 light profile. Real galaxies, however, are now known to have a range of different light-profile shapes that scale with mass. Consequent…

2005 Monthly Notices of the Royal Astronomical Society
eHST 100
A model of the Alfvén speed in the solar corona
DOI: 10.1051/0004-6361:20042169 Bibcode: 2005A&A...435.1123W

Mann, G.; Warmuth, A.

We present an analytic model of the Alfvén speed vA in the solar corona. The coronal magnetic field is modeled by a radial component representing the global field and by a dipole representing an active region. The free parameters of the model are constrained by actual observations of solar magnetic fields and coronal electron densities.…

2005 Astronomy and Astrophysics
SOHO 99
X-Ray/Ultraviolet Campaign on the Mrk 279 AGN Outflow: Constraining Inhomogeneous Absorber Models
DOI: 10.1086/425560 Bibcode: 2005ApJ...620..665A

Kriss, Gerard A.; Kaastra, Jelle; Korista, Kirk T. +3 more

We investigate the applicability of inhomogeneous absorber models in the formation of active galactic nucleus outflow absorption troughs. The models we explore are limited to monotonic gradients of absorbing column densities in front of a finite emission source. Our main finding is that simple power-law and Gaussian distributions are hard-pressed …

2005 The Astrophysical Journal
eHST 99
Near-infrared (0.8-4.0 µm) spectroscopy of Mimas, Enceladus, Tethys, and Rhea
DOI: 10.1051/0004-6361:20042482 Bibcode: 2005A&A...435..353E

Brown, R. H.; Emery, J. P.; Burr, D. M. +2 more

Spectral measurements from the ground in the time leading up to the Cassini mission at Saturn provide important context for the interpretation of the forthcoming spacecraft data. Whereas ground-based observations cannot begin to approach the spatial scales Cassini will achieve, they do possess the benefits of better spectral resolution, a broader …

2005 Astronomy and Astrophysics
Cassini 99
Far-Ultraviolet Spectroscopy of Magnetic Cataclysmic Variables
DOI: 10.1086/427914 Bibcode: 2005ApJ...622..589A

Szkody, Paula; Sion, Edward M.; Gänsicke, Boris T. +4 more

We have obtained Hubble Space Telescope (HST) STIS data for a total of 11 polars as part of a program aimed at compiling a homogeneous database of high-quality far-ultraviolet (FUV) spectra for a large number of cataclysmic variables (CVs). Of the 11 polars, eight were found in a state of low accretion activity (V347 Pav, VV Pup, V834 Cen, BL Hyi,…

2005 The Astrophysical Journal
eHST 98
Turbulence-driven Solar Wind Heating and Energization of Pickup Protons in the Outer Heliosphere
DOI: 10.1086/428609 Bibcode: 2005ApJ...623..502I

Isenberg, Philip A.

We improve and extend the ``dominant turbulence'' model of Isenberg et al., which describes the turbulent heating of the distant solar wind by the dissipation of wave energy generated by the isotropization of interstellar pickup protons. We first modify some of the detailed expressions in Isenberg et al. to fully incorporate the effects of wave di…

2005 The Astrophysical Journal
SOHO 98
X-rays from accretion shocks in T Tauri stars: The case of BP Tau
DOI: 10.1051/0004-6361:200500014 Bibcode: 2005A&A...432L..35S

Schmitt, J. H. M. M.; Ness, J. -U.; Robrade, J. +2 more

We present an XMM-Newton observation of the classical T Tauri star BP Tau. In the XMM-Newton RGS spectrum the O vii triplet is clearly detected with a very weak forbidden line indicating high plasma densities and/or a high UV flux environment. At the same time concurrent UV data point to a small hot spot filling factor suggesting an accretion funn…

2005 Astronomy and Astrophysics
XMM-Newton 98
Ly-α and ultraviolet emission from high-redshift gamma-ray burst hosts: to what extent do gamma-ray bursts trace star formation?
DOI: 10.1111/j.1365-2966.2005.09289.x Bibcode: 2005MNRAS.362..245J

Östlin, G.; Jóhannesson, G.; Watson, D. +9 more

We report the result of a search for Lyα emission from the host galaxies of the gamma-ray bursts (GRBs) 030226 (z= 1.986), 021004 (z= 2.335) and 020124 (z= 3.198). We find that the host galaxy of GRB 021004 is an extended (around 8 kpc) strong Lyα emitter with a rest-frame equivalent width (EW) of 68+12-11Å, and a star format…

2005 Monthly Notices of the Royal Astronomical Society
eHST 98
Local Correlation Tracking and the Magnetic Induction Equation
DOI: 10.1086/497633 Bibcode: 2005ApJ...632L..53S

Schuck, P. W.

Recently, local correlation tracking has been applied to magnetograms to estimate photospheric velocities. This Letter demonstrates that local correlation tracking is inconsistent with the magnetic induction equation, which governs the temporal evolution of the photospheric magnetograms. A modified formulation, consistent with the magnetic inducti…

2005 The Astrophysical Journal
SOHO 98