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Kinematics and stellar populations of the dwarf elliptical galaxy IC 3653
DOI: 10.1111/j.1365-2966.2007.11549.x Bibcode: 2007MNRAS.376.1033C

Afanasiev, V. L.; Chilingarian, I. V.; Sil'Chenko, O. K. +1 more

We present the first 3D observations of a diffuse elliptical galaxy (dE). The good quality data (S/N up to 40) reveal the kinematical signature of an embedded stellar disc, reminiscent of what is commonly observed in elliptical galaxies, though similarity of their origins is questionable. Colour map built from Hubble Space Telescope Advanced Camer…

2007 Monthly Notices of the Royal Astronomical Society
eHST 105
Slipping Magnetic Reconnection in Coronal Loops
DOI: 10.1126/science.1146143 Bibcode: 2007Sci...318.1588A

Golub, Leon; DeLuca, Edward E.; Narukage, Noriyuki +6 more

Magnetic reconnection of solar coronal loops is the main process that causes solar flares and possibly coronal heating. In the standard model, magnetic field lines break and reconnect instantaneously at places where the field mapping is discontinuous. However, another mode may operate where the magnetic field mapping is continuous but shows steep …

2007 Science
Hinode SOHO 104
A New Measurement of the Stellar Mass Density at z~5: Implications for the Sources of Cosmic Reionization
DOI: 10.1086/511325 Bibcode: 2007ApJ...659...84S

Bunker, A. J.; Stark, D. P.; Ellis, R. S. +2 more

We present a new measurement of the integrated stellar mass per comoving volume at redshift 5 determined via spectral energy fitting drawn from a sample of 214 photometrically selected galaxies with z'850LP<26.5 in the southern GOODS field. Following recent procedures introduced by Eyles et al., we estimate stellar masses …

2007 The Astrophysical Journal
eHST 104
X-rays from solar system objects
DOI: 10.1016/j.pss.2006.11.009 Bibcode: 2007P&SS...55.1135B

Snowden, Steven L.; Bhardwaj, Anil; Branduardi-Raymont, Graziella +11 more

During the last few years our knowledge about the X-ray emission from bodies within the solar system has significantly improved. Several new solar system objects are now known to shine in X-rays at energies below 2 keV. Apart from the Sun, the known X-ray emitters now include planets (Venus, Earth, Mars, Jupiter, and Saturn), planetary satellites …

2007 Planetary and Space Science
XMM-Newton 104
RPC-MIP: the Mutual Impedance Probe of the Rosetta Plasma Consortium
DOI: 10.1007/s11214-006-9005-1 Bibcode: 2007SSRv..128..713T

Schmidt, W.; Eriksson, A.; Décréau, P. M. E. +18 more

The main objective of the Mutual Impedance Probe (MIP), part of the Rosetta Plasma Consortium (RPC), is to measure the electron density and temperature of Comet 67P/Churyumov-Gerasimenko’s coma, in particular inside the contact surface. Furthermore, MIP will determine the bulk velocity of the ionised outflowing atmosphere, define the spectral dist…

2007 Space Science Reviews
Rosetta 104
Constraining the Equation of State of Supranuclear Dense Matter from XMM-Newton Observations of Neutron Stars in Globular Clusters
DOI: 10.1086/522877 Bibcode: 2007ApJ...671..727W

Webb, Natalie A.; Barret, Didier

We report on the detailed modeling of the X-ray spectra of three likely neutron stars. The neutron stars, observed with XMM-Newton, are found in three quiescent X-ray binaries in the globular clusters: ω Cen, M13, and NGC 2808. Whether they are accreting at very low rates or radiating energy from an accretion-heated core, their X-ray spectra are e…

2007 The Astrophysical Journal
XMM-Newton 104
First Space-Based Microlens Parallax Measurement: Spitzer Observations of OGLE-2005-SMC-001
DOI: 10.1086/518536 Bibcode: 2007ApJ...664..862D

Bennett, D. P.; Griest, K.; Reach, W. T. +20 more

We combine Spitzer and ground-based observations to measure the microlens parallax of OGLE-2005-SMC-001, the first such space-based determination since S. Refsdal proposed the idea in 1966. The parallax measurement yields a projected velocity v∼~230 km s-1, the typical value expected for halo lenses, but an order of magnitude smaller th…

2007 The Astrophysical Journal
eHST 104
RPC-ICA: The Ion Composition Analyzer of the Rosetta Plasma Consortium
DOI: 10.1007/s11214-006-9031-z Bibcode: 2007SSRv..128..671N

Kallio, E.; Fedorov, A.; Koskinen, H. +9 more

The Ion Composition Analyzer (ICA) is part of the Rosetta Plasma Consortium (RPC). ICA is designed to measure the three-dimensional distribution function of positive ions in order to study the interaction between the solar wind and cometary particles. The instrument has a mass resolution high enough to resolve the major species such as protons, he…

2007 Space Science Reviews
Rosetta 104
The first observation of AX J1749.1-2733 in a bright X-ray state—Another fast transient revealed by INTEGRAL
DOI: 10.1134/S1063773707030024 Bibcode: 2007AstL...33..149G

Sunyaev, R. A.; Grebenev, S. A.

An intense outburst of hard radiation (with a peak flux of ∼50 mCrab) was detected from the X-ray transient AX J1749.1-2733 by the IBIS/ISGRI gamma-ray telescope onboard the INTEGRAL observatory when the Galactic center field was monitored on September 8 10, 2003. Previously, this source had never been observed in a bright X-ray state. During the …

2007 Astronomy Letters
INTEGRAL 104
The PN.S Elliptical Galaxy Survey: Data Reduction, Planetary Nebula Catalog, and Basic Dynamics for NGC 3379
DOI: 10.1086/518358 Bibcode: 2007ApJ...664..257D

Freeman, K. C.; Capaccioli, M.; Napolitano, N. R. +9 more

We present results from Planetary Nebula Spectrograph (PN.S) observations of the elliptical galaxy NGC 3379 and a description of the data reduction pipeline. We detected 214 planetary nebulae, of which 191 are ascribed to NGC 3379 and 23 to the companion galaxy NGC 3384. Comparison with data from the literature shows that the PN.S velocities have …

2007 The Astrophysical Journal
eHST 103