Search Publications

Ion densities and velocities in the inner plasma torus of Saturn
DOI: 10.1016/j.pss.2012.09.016 Bibcode: 2012P&SS...73..151H

Persoon, A. M.; Wahlund, J. -E.; Morooka, M. W. +1 more

We present plasma data from the Cassini Radio and Plasma Wave Science (RPWS) Langmuir probe (LP), mapping the ion density and velocity of Saturn's inner plasma torus. Data from 129 orbits, recorded during the period from the 1st of February 2005 to the 27th of June 2010, are used to map the extension of the inner plasma torus. The dominant part of…

2012 Planetary and Space Science
Cassini 38
Infrared and Hard X-Ray Diagnostics of Active Galactic Nucleus Identification from the Swift/BAT and AKARI All-sky Surveys
DOI: 10.1088/0004-637X/753/2/104 Bibcode: 2012ApJ...753..104M

Stawarz, Ł.; Gandhi, P.; Oyabu, S. +8 more

We combine data from two all-sky surveys in order to study the connection between the infrared and hard X-ray (>10 keV) properties for local active galactic nuclei (AGNs). The Swift Burst Alert Telescope all-sky survey provides an unbiased, flux-limited selection of hard X-ray-detected AGNs. Cross-correlating the 22 month hard X-ray survey with…

2012 The Astrophysical Journal
AKARI Suzaku 38
Chemical Analysis of a Diffuse Cloud along a Line of Sight toward W51: Molecular Fraction and Cosmic-Ray Ionization Rate
DOI: 10.1088/0004-637X/758/2/83 Bibcode: 2012ApJ...758...83I

Menten, K. M.; Gerin, M.; Goicoechea, J. R. +4 more

Absorption lines from the molecules OH+, H2O+, and H+ 3 have been observed in a diffuse molecular cloud along a line of sight near W51 IRS2. We present the first chemical analysis that combines the information provided by all three of these species. Together, OH+ and H2O<…

2012 The Astrophysical Journal
Herschel 38
A Chandra view of the z = 1.62 galaxy cluster IRC-0218A
DOI: 10.1051/0004-6361/201118169 Bibcode: 2012A&A...540A...4P

Papovich, C.; Pierre, M.; Clerc, N. +3 more

Context. Very few z > 1.5 clusters of galaxies are currently known. It is important to study the properties of galaxies in these clusters and the intra-cluster medium and, furthermore, to cross-check the reliability of the various mass estimates. This will help to clarify the process of structure formation and how distant clusters may be used t…

2012 Astronomy and Astrophysics
XMM-Newton 38
The quasi-biennial periodicity (QBP) in velocity and intensity helioseismic observations. The seismic QBP over solar cycle 23
DOI: 10.1051/0004-6361/201118057 Bibcode: 2012A&A...539A.135S

García, R. A.; Roth, M.; Finsterle, W. +4 more


Aims: We looked for signatures of quasi-biennial periodicity (QBP) over different phases of solar cycle by means of acoustic modes of oscillation. Low-degree p-mode frequencies are shown to be sensitive to changes in magnetic activity due to the global dynamo. Recently there has been reported evidence of two-year variations in p-mode frequenc…

2012 Astronomy and Astrophysics
SOHO 38
Automated classification of Hipparcos unsolved variables
DOI: 10.1111/j.1365-2966.2012.21752.x Bibcode: 2012MNRAS.427.2917R

Rimoldini, L.; Mowlavi, N.; Nienartowicz, K. +14 more

We present an automated classification of stars exhibiting periodic, non-periodic and irregular light variations. The Hipparcos catalogue of unsolved variables is employed to complement the training set of periodic variables of Dubath et al. with irregular and non-periodic representatives, leading to 3881 sources in total which describe 24 variabi…

2012 Monthly Notices of the Royal Astronomical Society
Hipparcos 38
Asteroid (2867) Steins: Shape, topography and global physical properties from OSIRIS observations
DOI: 10.1016/j.icarus.2012.07.035 Bibcode: 2012Icar..221.1089J

Jorda, L.; Lamy, P. L.; Groussin, O. +4 more

The Rosetta spacecraft flew by Asteroid (2867) Steins on 5 September 2008, allowing the onboard OSIRIS cameras to collect the first images of an E-type asteroid. We implemented several three-dimensional reconstruction techniques to retrieve its shape. Limb profiles, combined with stereo control points, were used to reconstruct an approximate shape…

2012 Icarus
Rosetta 38
OPACOS: OVRO Post-AGB CO (1-0) Emission Survey. I. Data and Derived Nebular Parameters
DOI: 10.1088/0067-0049/203/1/16 Bibcode: 2012ApJS..203...16S

Sahai, R.; Sánchez Contreras, C.

We have performed interferometric observations of the 12CO (J = 1-0) emission in a sample of 27 objects spanning different evolutionary stages from the late asymptotic giant branch (late-AGB), through the post-AGB (pAGB) phase, and to the planetary nebula (PN) stage, but dominated by pAGB objects and young PNs (>=81%). In this paper …

2012 The Astrophysical Journal Supplement Series
AKARI eHST 38
An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. Application to XTE J1118+480
DOI: 10.1051/0004-6361/201118106 Bibcode: 2012A&A...538A..97V

Romero, G. E.; Vila, G. S.; Casco, N. A.

Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observed electromagnetic spectrum, is a complex inverse problem.
Aims: We aim to improve our understanding of the mechanisms operating in relativistic jets by modeling their broadband electromagnetic spectrum.
Methods: We develop an inhomogeneous…

2012 Astronomy and Astrophysics
eHST 38
Early-type Galaxies with Tidal Debris and Their Scaling Relations in the Spitzer Survey of Stellar Structure in Galaxies (S4G)
DOI: 10.1088/0004-637X/753/1/43 Bibcode: 2012ApJ...753...43K

Ho, Luis C.; Erroz-Ferrer, Santiago; Schinnerer, Eva +21 more

Tidal debris around galaxies can yield important clues on their evolution. We have identified tidal debris in 11 early-type galaxies (T <= 0) from a sample of 65 early types drawn from the Spitzer Survey of Stellar Structure in Galaxies (S4G). The tidal debris includes features such as shells, ripples, and tidal tails. A variety of t…

2012 The Astrophysical Journal
eHST 38