Search Publications

Structures induced by small moonlets in Saturn's rings: Implications for the Cassini Mission
DOI: 10.1029/2005GL022506 Bibcode: 2005GeoRL..3211205S

Seiß, M.; Spahn, F.; Sremčević, M. +1 more

Particle simulations are carried out to study density features caused by small moonlets embedded in a dense planetary ring. The creation of a ``propeller'' like structure is found together with adjacent density wakes. Both features are clear indications for the existence of moonlets in the rings. We confirmed that the propeller scales with the Hil…

2005 Geophysical Research Letters
Cassini 37
The connection between ultraviolet and X-ray outflows in active galactic nuclei: the case of PDS 456
DOI: 10.1111/j.1745-3933.2005.00038.x Bibcode: 2005MNRAS.360L..25O

Simpson, Chris; O'Brien, Paul T.; Reeves, James N. +1 more

High-velocity outflows from active galactic nuclei are a well-known phenomenon in terms of the broad absorption lines seen in the ultraviolet/optical. More recently, similar, possibly related, outflows have been reported in the X-ray. The most extreme example is seen in the nearby, luminous QSO PDS 456, which displays a massive, high-velocity (500…

2005 Monthly Notices of the Royal Astronomical Society
eHST 37
XMM-Newton View of the Ultraluminous X-Ray Sources in M51
DOI: 10.1086/497356 Bibcode: 2005ApJ...635..198D

Dewangan, Gulab C.; Griffiths, Richard E.; Miyaji, Takamitsu +2 more

We present results based on XMM-Newton observations of the nearby spiral galaxy M51 (NGC 5194 and NGC 5195). We confirm the presence of the seven known ultraluminous X-ray sources (ULXs) with luminosities exceeding the Eddington luminosity for a 10 Msolar black hole, a low-luminosity active galactic nucleus (LLAGN) with 2-10 keV luminos…

2005 The Astrophysical Journal
XMM-Newton 37
Spatially resolved spectroscopy of the E+A galaxies in the z= 0.32 cluster AC 114
DOI: 10.1111/j.1365-2966.2005.08983.x Bibcode: 2005MNRAS.359.1421P

Kuntschner, Harald; Bekki, Kenji; Colless, Matthew +5 more

We present spatially resolved intermediate-resolution spectroscopy of a sample of 12 E+A galaxies in the z= 0.32 rich galaxy cluster AC 114, obtained with the FLAMES multi-integral field unit system on the Very Large Telescope (VLT) of the European Southern Observatory. Previous integrated spectroscopy of all these galaxies by Couch & Sharples…

2005 Monthly Notices of the Royal Astronomical Society
eHST 37
A New Technique for Deriving Prominence Mass from SOHO/EIT Fe XII (19.5 Nanometers) Absorption Features
DOI: 10.1086/425975 Bibcode: 2005ApJ...618..524G

Gilbert, Holly R.; Holzer, Thomas E.; MacQueen, R. M.

It is presently unclear what role prominences play in the initiation and dynamics of coronal mass ejections (CMEs), although erupting prominences are strongly correlated with CMEs. The masses of prominences involved in CMEs are not generally measured, but the accurate determination of such masses may help in assessing the dynamical importance of p…

2005 The Astrophysical Journal
SOHO 36
Are radio galaxies and quiescent galaxies different? Results from the analysis of HST brightness profiles
DOI: 10.1051/0004-6361:20042529 Bibcode: 2005A&A...439..487D

Capetti, A.; Morganti, R.; de Ruiter, H. R. +3 more

We present a study of the optical brightness profiles of early type galaxies, using a number of samples of radio galaxies and optically selected elliptical galaxies. For the radio galaxy samples - B2 of Fanaroff-Riley type I and 3C of Fanaroff-Riley type II - we determined a number of parameters that describe a "Nuker-law" profile, which were comp…

2005 Astronomy and Astrophysics
eHST 36
Evolution in the Cluster Early-Type Galaxy Size-Surface Brightness Relation at z~=1
DOI: 10.1086/430248 Bibcode: 2005ApJ...626..809H

Demarco, R.; Infante, L.; Zheng, W. +41 more

We investigate the evolution in the distribution of surface brightness, as a function of size, for elliptical and S0 galaxies in the two clusters RDCS J1252.9-2927 (z=1.237) and RX J0152.7-1357 (z=0.837). We use multicolor imaging with the Advanced Camera for Surveys on the Hubble Space Telescope to determine these sizes and surface brightnesses. …

2005 The Astrophysical Journal
eHST 36
Calibration of the Planetary Fourier Spectrometer short wavelength channel
DOI: 10.1016/j.pss.2004.12.007 Bibcode: 2005P&SS...53..975G

Piccioni, G.; Grassi, D.; Moshkin, B. E. +18 more

The Planetary Fourier Spectrometer (PFS) experiment on board the Mars Express mission has two channels covering the 1.2-5.5 µm short wavelength channel (SWC) and the 5.5-45 µm (LWC). The SWC measures part of the thermal emission spectrum and the solar reflected spectrum of Mars between 1700 and 8200 cm -1 with a spectral res…

2005 Planetary and Space Science
MEx 36
Coronal properties of G-type stars in different evolutionary phases
DOI: 10.1051/0004-6361:20041739 Bibcode: 2005A&A...432..671S

Pallavicini, R.; Peres, G.; Maggio, A. +1 more

We report on the analysis of XMM-Newton observations of three G-type stars in very different evolutionary phases: the weak-lined T Tauri star HD 283572, the Zero Age Main Sequence star EK Dra and the Hertzsprung-gap giant star 31 Com. They all have high X-ray luminosity (~1031 erg…

2005 Astronomy and Astrophysics
XMM-Newton 36
X-Ray Spectroscopy of Candidate Ultracompact X-Ray Binaries
DOI: 10.1086/430633 Bibcode: 2005ApJ...627..926J

Chakrabarty, Deepto; Juett, Adrienne M.

We present high-resolution spectroscopy of the neutron star/low-mass X-ray binaries (LMXBs) 4U 1850-087 and 4U 0513-40 as part of our continuing study of known and candidate ultracompact binaries. The LMXB 4U 1850-087 is one of four systems in which we had previously inferred an unusual Ne/O ratio in the absorption along the line of sight, most li…

2005 The Astrophysical Journal
XMM-Newton 36