Search Publications

Statistical study of coronal mass ejection source locations: 2. Role of active regions in CME production
DOI: 10.1029/2011JA016844 Bibcode: 2011JGRA..11612108C

Wang, Yuming; Shen, Chenglong; Wang, S. +3 more

This is the second paper of the statistical study of coronal mass ejection (CME) source locations, in which the relationship between CMEs and active regions (ARs) is statistically studied on the basis of the information of CME source locations and the ARs automatically extracted from magnetic synoptic charts of Michelson Doppler Imager (MDI) durin…

2011 Journal of Geophysical Research (Space Physics)
SOHO 25
Gas temperature profiles in galaxy clusters with Swift XRT: observations and capabilities to map near R200
DOI: 10.1051/0004-6361/201015966 Bibcode: 2011A&A...528A.102M

Moretti, A.; Molendi, S.; Gastaldello, F. +1 more


Aims: We investigate the possibility of using the X-ray telescope (XRT) on board the Swift satellite to improve the current accuracy of the intra-cluster medium (ICM) temperature measurements in the region close to the virial radius of nearby clusters.
Methods: We present the spectral analysis of the Swift XRT observations of 6 galaxy cl…

2011 Astronomy and Astrophysics
Suzaku 25
On the Spin-down and Magnetic Field of the X-ray Pulsar 1E 1207.4-5209
DOI: 10.1088/2041-8205/733/2/L28 Bibcode: 2011ApJ...733L..28H

Gotthelf, E. V.; Halpern, J. P.

We analyze all of the archival X-ray timing data from the years 2000-2008 on the weakly magnetized central compact object (CCO) pulsar 1E 1207.4-5209 in an attempt to measure its dipole magnetic field strength via spin-down. because most of these observations were not planned for the purpose of phase-coherent timing, the resulting ephemeris is not…

2011 The Astrophysical Journal
XMM-Newton 25
Hot electrons as tracers of large-scale structure of magnetotail current sheets
DOI: 10.1029/2011GL047979 Bibcode: 2011GeoRL..3814102A

Petrukovich, A. A.; Zelenyi, L. M.; Nakamura, R. +1 more

This paper is devoted to the investigation of the vertical electron temperature distribution in thin currents sheets of the Earth magnetotail. The dependence of electron temperature on magnetic field Te(Bx) is examined for 62 thin currents sheet crossings by the Cluster spacecraft. The profiles Te(Bx) ar…

2011 Geophysical Research Letters
Cluster 25
Nonlinear Force-Free Reconstruction of the Global Solar Magnetic Field: Methodology
DOI: 10.1007/s11207-011-9713-x Bibcode: 2011SoPh..269..351C

Contopoulos, I.; Kalapotharakos, C.; Georgoulis, M. K.

We present a novel numerical method that allows the calculation of nonlinear force-free magnetostatic solutions above a boundary surface on which only the distribution of the normal magnetic field component is given. The method relies on the theory of force-free electrodynamics and applies directly to the reconstruction of the solar coronal magnet…

2011 Solar Physics
SOHO 25
Discovery of the correspondence between intra-cluster radio emission and a high pressure region detected through the Sunyaev-Zel'dovich effect
DOI: 10.1051/0004-6361/201117788 Bibcode: 2011A&A...534L..12F

Croston, J. H.; Bourdin, H.; Mazzotta, P. +9 more

We analyzed new 237 MHz and 614 MHz GMRT data of the most X-ray luminous galaxy cluster, RX J1347-1145. Our radio results are compared with the MUSTANG 90 GHz Sunyaev-Zel'dovich effect map and with re-processed Chandra and XMM-Newton archival data of this cluster. We point out for the first time in an unambiguous way the correspondence between a r…

2011 Astronomy and Astrophysics
XMM-Newton 25
Rotational modeling of Hyperion
DOI: 10.1007/s10569-011-9337-3 Bibcode: 2011CeMDA.110....1H

Thomas, Peter C.; Harbison, Rebecca A.; Nicholson, Philip C.

Saturn's moon, Hyperion, is subject to strongly-varying solid body torques from its primary and lacks a stable spin state resonant with its orbital frequency. In fact, its rotation is chaotic, with a Lyapunov timescale on the order of 100 days. In 2005, Cassini made three close passes of Hyperion at intervals of 40 and 67 days, when the moon was i…

2011 Celestial Mechanics and Dynamical Astronomy
Cassini 25
An optical/NIR survey of globular clusters in early-type galaxies. I. Introduction and data reduction procedures
DOI: 10.1051/0004-6361/201015681 Bibcode: 2011A&A...525A..19C

Larsen, S. S.; Kuntschner, H.; Chies-Santos, A. L. +3 more

Context. The combination of optical and near-infrared (NIR) colours has the potential to break the age/metallicity degeneracy and offers a better metallicity sensitivity than optical colours alone. Previous tudies of extragalactic globular clusters (GCs) with this colour combination, however, have suffered from small samples or have been restricte…

2011 Astronomy and Astrophysics
eHST 25
Thermal properties of the asteroid (2867) Steins as observed by VIRTIS/Rosetta
DOI: 10.1051/0004-6361/201116529 Bibcode: 2011A&A...531A.168L

Erard, S.; Drossart, P.; Capaccioni, F. +6 more

Context. To investigate thermal properties of the small asteroid (2867) Steins, we analyzed its surface thermal emission measured by the VIRTIS instrument during the Rosetta spacecraft (ESA) flyby that occurred in September 2008. VIRTIS performed the first thermal mapping of an asteroid surface.
Aims: We determine the thermal properties of di…

2011 Astronomy and Astrophysics
Rosetta 25
Fokker-Planck Models for M15 Without a Central Black Hole: The Role of the Mass Function
DOI: 10.1088/0004-637X/732/2/67 Bibcode: 2011ApJ...732...67M

Cohn, Haldan N.; Lugger, Phyllis M.; Murphy, Brian W.

We have developed a set of dynamically evolving Fokker-Planck models for the collapsed-core globular star cluster M15, which directly address the issue of whether a central black hole is required to fit Hubble Space Telescope (HST) observations of the stellar spatial distribution and kinematics. As in our previous work reported by Dull et al., we …

2011 The Astrophysical Journal
eHST 25