Search Publications

Is Pre-Eruptive Null Point Reconnection Required for Triggering Eruptions?
DOI: 10.1007/s11207-006-0173-7 Bibcode: 2006SoPh..237...85L

Li, Hui; Aulanier, Guillaume; Schmieder, Brigitte +1 more

We study the magnetic field evolution and topology of the active region NOAA 10486 before the 3B/X1.2 flare of October 26, 2003, using observational data from the French-Italian THEMIS telescope, the Michelson Doppler Imager (MDI) onboard Solar and Heliospheric Observatory (SOHO), the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observat…

2006 Solar Physics
SOHO 21
A short review of relativistic iron lines from stellar-mass black holes
DOI: 10.1002/asna.200610680 Bibcode: 2006AN....327..997M

Miller, J. M.

% In this contribution, I briefly review recent progress in detecting and measuring the properties of relativistic iron lines observed in stellar-mass black hole systems, and the aspects of these lines that are most relevant to studies of similar lines in Seyfert-1 AGN. In particular, the lines observed in stellar-mass black holes are not complica…

2006 Astronomische Nachrichten
XMM-Newton 21
The Interstellar N/O Abundance Ratio: Evidence for Local Infall?
DOI: 10.1086/507451 Bibcode: 2006ApJ...647L.115K

Meyer, David M.; Lauroesch, James T.; Knauth, David C.

Sensitive measurements of the interstellar gas-phase oxygen abundance have revealed a slight oxygen deficiency (~15%) toward stars within 500 pc of the Sun as compared to more distant sight lines. Recent FUSE observations of the interstellar gas-phase nitrogen abundance indicate larger variations, but no trends with distance were reported due to t…

2006 The Astrophysical Journal
eHST 21
Next generation of pnCCDs for X-ray spectroscopy and imaging
DOI: 10.1016/j.nima.2006.05.268 Bibcode: 2006NIMPA.568..141M

Meidinger, Norbert; Strüder, Lothar; Herrmann, Sven +10 more

A special type of charge-coupled device, the pnCCD, has been developed in the nineties as focal-plane detector for the X-ray astronomy mission XMM-Newton of the European Space Agency. The pnCCD detector has been in operation since the satellite launch in 1999. It is performing up to date spectroscopy of X-rays in combination with imaging and high …

2006 Nuclear Instruments and Methods in Physics Research A
XMM-Newton 21
Shock-cloud interaction in the Vela SNR. II. Hydrodynamic model
DOI: 10.1051/0004-6361:20065738 Bibcode: 2006A&A...458..213M

Miceli, M.; Bocchino, F.; Orlando, S. +1 more

Context: .In the framework of the study of the X-ray and optical emission in supernova remnants we focus on an isolated X-ray knot in the northern rim of the Vela SNR (Vela FilD), whose X-ray emission has been studied and discussed in Paper I.
Aims: .We aim at understanding the physical origin of the X-ray and optical emission in FilD, at unde…

2006 Astronomy and Astrophysics
XMM-Newton 21
Energetic Neutral Atoms (ENA) at Mars: Properties of the hydrogen atoms produced upstream of the martian bow shock and implications for ENA sounding technique around non-magnetized planets
DOI: 10.1016/j.icarus.2005.12.019 Bibcode: 2006Icar..182..448K

Coates, A. J.; Kallio, E.; Fedorov, A. +43 more

We have studied the interaction of fast solar wind hydrogen atoms with the martian atmosphere by a three-dimensional Monte Carlo simulation. These energetic neutral hydrogen atoms, H-ENAs, are formed upstream of the martian bow shock. Both H-ENAs scattered and non-scattered from the martian atmosphere/exosphere were studied. The colliding H-ENAs w…

2006 Icarus
MEx 21
Examining the Seyfert-Starburst Connection with Arcsecond-Resolution Radio Continuum Observations
DOI: 10.1086/499037 Bibcode: 2006AJ....131..701L

Ryder, Stuart D.; Laine, Seppo; Beck, Rainer +2 more

We compare the arcsecond-scale circumnuclear radio continuum properties of five Seyfert and five starburst galaxies, concentrating on the search for any structures that could imply a spatial or causal connection between the nuclear activity and a circumnuclear starburst ring. No evidence is found in the radio emission for a link between the trigge…

2006 The Astronomical Journal
eHST 21
Oxygen-rich disk in the V778 Cygni system resolved
DOI: 10.1051/0004-6361:20053782 Bibcode: 2006A&A...452..561S

Szczerba, R.; Richards, A. M. S.; Poutanen, J. +3 more

Aims.Various scenarios have been proposed to explain the presence of silicate features associated with carbon stars, such as V778 Cyg. We have attempted to constrain these theories by means of mapping water maser emission from V778 Cyg.
Methods: .The 22 GHz water maser emission from this star has been mapped using MERLIN wit…

2006 Astronomy and Astrophysics
Hipparcos 21
Double-barred galaxies at intermediate redshifts: a feasibility study
DOI: 10.1111/j.1365-2966.2006.10493.x Bibcode: 2006MNRAS.370..477L

Lisker, Thorsten; Debattista, Victor P.; Ferreras, Ignacio +1 more

Despite the increasing number of studies of barred galaxies at intermediate and high redshifts, double-barred (S2B) systems have only been identified in the nearby (z <= 0.04) universe thus far. In this feasibility study, we demonstrate that the detection and analysis of S2Bs is possible at intermediate redshifts (0.1 <~ z <~ 0.5) with th…

2006 Monthly Notices of the Royal Astronomical Society
eHST 21
The Blue Straggler Population of the Globular Cluster M5: Comparison with M3
DOI: 10.1086/505481 Bibcode: 2006ApJ...648.1026W

Warren, Steven R.; Bolte, Michael; Sandquist, Eric L.

We have surveyed the blue straggler star population of the Galactic globular cluster M5 using high-resolution images of the core along with wide-field ground-based images reaching to more than 19 core radii. To gauge M5's relative efficiency of producing stragglers, we compared our sample to five studies of other globular clusters. Using a ``brigh…

2006 The Astrophysical Journal
eHST 21