Search Publications

Dynamo regime transition among Sun-like stars in M 34. A time evolution model of X-ray activity on the main sequence
DOI: 10.1051/0004-6361/201219823 Bibcode: 2012A&A...546A.117G

Gondoin, P.

Context. The X-ray emission from late-type stars in open clusters exhibits two kinds of dependences on stellar rotation. While fast rotators have a relatively constant X-ray emission level, slower rotators show a decline of their X-ray emission with decreasing rotation rate. The physical significance of the transition between these two X-ray emiss…

2012 Astronomy and Astrophysics
XMM-Newton 22
Nonlinear Force-free Modeling of a Three-dimensional Sigmoid Observed on the Sun
DOI: 10.1088/0004-637X/747/1/65 Bibcode: 2012ApJ...747...65I

Choe, G. S.; Inoue, S.; Magara, T. +1 more

In this work, we analyze the characteristics of the three-dimensional magnetic structure of a sigmoid observed over an active region (AR 10930) and followed by X-class flares. This is accomplished by combining a nonlinear force-free field (NLFFF) model of a coronal magnetic field and the high-resolution vector-field measurement of a photospheric m…

2012 The Astrophysical Journal
Hinode SOHO 21
Analysis of GRB 080319B and GRB 050904 within the Fireshell Model: Evidence for a Broader Spectral Energy Distribution
DOI: 10.1088/0004-637X/756/1/16 Bibcode: 2012ApJ...756...16P

Izzo, L.; Bernardini, M. G.; Patricelli, B. +5 more

The observation of GRB 080319B, with an isotropic energy E iso = 1.32 × 1054 erg, and GRB 050904, with E iso = 1.04 × 1054 erg, offers the possibility of studying the spectral properties of the prompt radiation of two of the most energetic gamma-ray bursts (GRBs). This allows us to probe the validity of …

2012 The Astrophysical Journal
INTEGRAL 21
Acoustic spectrum fitting for a large set of solar-like pulsators
DOI: 10.1111/j.1365-2966.2011.20184.x Bibcode: 2012MNRAS.420.2178B

Baudin, F.; Chaplin, W. J.; Elsworth, Y. +2 more

Asteroseismology provides the means both to constrain the global properties and to probe the internal structures of stars. Asteroseismic data are now available on large numbers of solar-type stars, thanks in particular to the CoRoT and Kepler space missions, and automated data-analysis pipelines are needed to provide efficient and timely results. …

2012 Monthly Notices of the Royal Astronomical Society
SOHO 21
Dielectric constant estimation of the uppermost Basal Unit layer in the martian Boreales Scopuli region
DOI: 10.1016/j.icarus.2012.03.011 Bibcode: 2012Icar..219..458L

Orosei, Roberto; Pettinelli, Elena; Mattei, Elisabetta +3 more

An electromagnetic inversion model has been applied to echoes from the subsurface sounding Shallow Radar (SHARAD) to retrieve the dielectric properties of the uppermost Basal Unit (BU) beneath the North Polar Layered Deposits of Mars. SHARAD data have been carefully selected to satisfy the assumption of the inversion model which requires a stratig…

2012 Icarus
MEx 21
A Hubble Space Telescope Treasury Study of Star-forming Regions in the Local Group. II. Young Stellar Populations in M31
DOI: 10.1088/0004-6256/144/5/142 Bibcode: 2012AJ....144..142B

Bianchi, Luciana; Hodge, Paul; Kang, Yongbeom +1 more

We studied the young stellar populations of 22 star-forming regions in the Andromeda galaxy (M31), with Hubble Space Telescope (HST) multi-band imaging from far-UV to I. The regions were selected from Galaxy Evolution Explorer (GALEX) wide-field far-UV imaging; they sample different environments and galactocentric distances from 6 to 22 kpc. They …

2012 The Astronomical Journal
eHST 21
A time-variable, phase-dependent emission line in the X-ray spectrum of the isolated neutron star RX J0822-4300
DOI: 10.1111/j.1745-3933.2011.01209.x Bibcode: 2012MNRAS.421L..72D

Caraveo, P. A.; Bignami, G. F.; Tiengo, A. +9 more

RX J0822-4300 is the central compact object associated with the Puppis A supernova remnant. Previous X-ray observations suggested RX J0822-4300 to be a young neutron star with a weak dipole field and a peculiar surface temperature distribution dominated by two antipodal spots with different temperatures and sizes. An emission line at 0.8 keV was a…

2012 Monthly Notices of the Royal Astronomical Society
XMM-Newton 21
12 Years of X-Ray Variability in M31 Globular Clusters, Including 8 Black Hole Candidates, as Seen by Chandra
DOI: 10.1088/0004-637X/757/1/40 Bibcode: 2012ApJ...757...40B

Murray, S. S.; Barnard, R.; Garcia, M.

We examined 134 Chandra observations of the population of X-ray sources associated with globular clusters (GCs) in the central region of M31. These are expected to be X-ray binary systems (XBs), consisting of a neutron star or black hole accreting material from a close companion. We created long-term light curves for these sources, correcting for …

2012 The Astrophysical Journal
XMM-Newton 21
Suzaku X-Ray Follow-up Observations of Seven Unassociated Fermi-LAT Gamma-Ray Sources at High Galactic Latitudes
DOI: 10.1088/0004-637X/747/1/64 Bibcode: 2012ApJ...747...64T

Cheung, C. C.; Guillemot, L.; Kataoka, J. +8 more

We report on our second-year campaign of X-ray follow-up observations of unidentified Fermi Large Area Telescope (LAT) γ-ray sources at high Galactic latitudes (|b| > 10°) using the X-ray Imaging Spectrometer on board the Suzaku X-ray Observatory. In this second year of the project, seven new targets were selected from the First Fermi-LAT Catal…

2012 The Astrophysical Journal
Suzaku 21
A statistical study of energy release and transport midway between the magnetic reconnection and initial dipolarization regions in the near-Earth magnetotail associated with substorm expansion onsets
DOI: 10.1029/2012JA017925 Bibcode: 2012JGRA..11711214M

Paterson, W. R.; Miyashita, Y.; Saito, Y. +3 more

Our previous study showed that the energy release associated with substorm expansion onsets is the most significant midway between the magnetic reconnection and initial dipolarization regions (-12 > X > -18 RE in the premidnight sector) in the magnetotail. In the present paper, we have statistically studied the substorm-associated…

2012 Journal of Geophysical Research (Space Physics)
Cluster 21