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Properties of Newly Formed Dust by SN 2006JC Based on Near- to Mid-Infrared Observation With AKARI
DOI: 10.1088/0004-637X/692/1/546 Bibcode: 2009ApJ...692..546S

Tanaka, M.; Ohyama, Y.; Matsuhara, H. +18 more

We present our latest results on near- to mid-infrared (MIR) observation of supernova (SN) 2006jc at 200 days after the discovery using the Infrared Camera (IRC) on board AKARI. The near-infrared (2-5 µm) spectrum of SN 2006jc is obtained for the first time and is found to be well interpreted in terms of the thermal emission from amorphous c…

2009 The Astrophysical Journal
AKARI 60
The secondary eclipse of CoRoT-1b
DOI: 10.1051/0004-6361/200912102 Bibcode: 2009A&A...506..353A

Mazeh, T.; Aigrain, S.; Alapini, A. +33 more

The transiting planet CoRoT-1b is thought to belong to the pM-class of planets, in which the thermal emission dominates in the optical wavelengths. We present a detection of its secondary eclipse in the CoRoT white channel data, whose response function goes from ~400 to ~1000 nm. We used two different filtering approaches, and several methods to e…

2009 Astronomy and Astrophysics
CoRoT 60
X-ray emission from the extended discs of spiral galaxies
DOI: 10.1111/j.1365-2966.2009.14464.x Bibcode: 2009MNRAS.394.1741O

Warwick, R. S.; Owen, R. A.

We present a study of the X-ray properties of a sample of six nearby late-type spiral galaxies based on XMM-Newton observations. Since our primary focus is on the linkage between X-ray emission and star formation in extended, extranuclear Galactic discs, we have selected galaxies with near face-on aspect and sufficient angular extent so as to be r…

2009 Monthly Notices of the Royal Astronomical Society
XMM-Newton 60
X-ray observations of PSR B1259-63 near the 2007 periastron passage
DOI: 10.1111/j.1365-2966.2009.15116.x Bibcode: 2009MNRAS.397.2123C

Takahashi, T.; Uchiyama, Y.; Aharonian, F. +2 more

PSR B1259-63 is a 48-ms radio pulsar in a highly eccentric 3.4-yr orbit with a Be star SS 2883. Unpulsed γ-ray, X-ray and radio emission components are observed from the binary system. It is likely that the collision of the pulsar wind with the anisotropic wind of the Be star plays a crucial role in the generation of the observed non-thermal emiss…

2009 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 60
A Self-Consistent Nonlinear Force-Free Solution for a Solar Active Region Magnetic Field
DOI: 10.1088/0004-637X/700/2/L88 Bibcode: 2009ApJ...700L..88W

Régnier, S.; Wheatland, M. S.

Nonlinear force-free solutions for the magnetic field in the solar corona constructed using photospheric vector magnetic field boundary data suffer from a basic problem: the observed boundary data are inconsistent with the nonlinear force-free model. Specifically, there are two possible choices of boundary conditions on vertical current provided b…

2009 The Astrophysical Journal
Hinode SOHO 60
High energy neutron and pion-decay gamma-ray emissions from solar flares
DOI: 10.1088/1674-4527/9/1/003 Bibcode: 2009RAA.....9...11C

Chupp, Edward L.; Ryan, James M.

Solar flare gamma-ray emissions from energetic ions and electrons have been detected and measured to GeV energies since 1980. In addition, neutrons produced in solar flares with 100 MeV to GeV energies have been observed at the Earth. These emissions are produced by the highest energy ions and electrons accelerated at the Sun and they provide our …

2009 Research in Astronomy and Astrophysics
INTEGRAL 60
Spectral and intensity variations of Galactic 26Al emission
DOI: 10.1051/0004-6361/200811175 Bibcode: 2009A&A...496..713W

Wang, W.; Strong, A. W.; Knödlseder, J. +9 more

Aims: Gamma-ray line emission from the radioactive decay of 26Al reflects nucleosynthesis in massive stars and supernovae. We use INTEGRAL 26Al measurements to characterize the distribution and characteristics of 26Al source regions throughout the Galaxy.
Methods: The spectrometer SPI aboard INTEGRAL has accumu…

2009 Astronomy and Astrophysics
INTEGRAL 60
Spitzer View of Young Massive Stars in the Large Magellanic Cloud H II Complex N 44
DOI: 10.1088/0004-637X/695/1/511 Bibcode: 2009ApJ...695..511C

Gordon, Karl D.; Chu, You-Hua; Gruendl, Robert A. +2 more

The H II complex N 44 in the Large Magellanic Cloud (LMC) provides an excellent site to perform a detailed study of star formation in a mild starburst, as it hosts three regions of star formation at different evolutionary stages, and it is not as complicated and confusing as the 30 Doradus giant H II region. We have obtained Spitzer Space Telescop…

2009 The Astrophysical Journal
eHST 60
Searching for modifications to the exponential radioactive decay law with the Cassini spacecraft
DOI: 10.1016/j.astropartphys.2009.02.005 Bibcode: 2009APh....31..267C

Cooper, Peter S.

Data from the power output of the radioisotope thermoelectric generators aboard the Cassini spacecraft are used to test the conjecture that small deviations observed in terrestrial measurements of the exponential radioactive decay law are correlated with the Earth-Sun distance. No significant deviations from exponential decay are observed over a r…

2009 Astroparticle Physics
Cassini 60
On the numerical modelling of VLF chorus dynamical spectra
DOI: 10.5194/angeo-27-2341-2009 Bibcode: 2009AnGeo..27.2341N

Santolik, O.; Nunn, D.; Rycroft, M. +1 more

This paper presents a study of the use of a one-dimensional Vlasov Hybrid Simulation (VHS) computer code to simulate the dynamical spectra (i.e. frequency versus time spectrograms) of ELF/VLF chorus signals (from ~a fraction to ~10 kHz). Recently excellent measurements of chorus have been made in the source region close to the geomagnetic equator …

2009 Annales Geophysicae
Cluster 60