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Evidence for the Disky Origin of Luminous Virgo Dwarf Ellipticals from the Kinematics of Their Globular Cluster Systems
DOI: 10.1088/0004-6256/137/6/5146 Bibcode: 2009AJ....137.5146B

Brodie, Jean P.; Beasley, Michael A.; Strader, Jay +1 more

We report evidence for dynamically significant rotation in the globular cluster systems of two luminous Virgo dwarf ellipticals, VCC1261 and VCC1528. Including previous results for VCC1087, the globular cluster systems of all three Virgo dwarf ellipticals studied in detail to date exhibit v rotlos>1. Taking the rotation …

2009 The Astronomical Journal
eHST 33
GRI: focusing on the evolving violent universe
DOI: 10.1007/s10686-008-9119-4 Bibcode: 2009ExA....23..121K

Knödlseder, Jürgen; Christensen, Finn; Bazzano, Angela +4 more

The gamma-ray imager (GRI) is a novel mission concept that will provide an unprecedented sensitivity leap in the soft gamma-ray domain by using for the first time a focusing lens built of Laue diffracting crystals. The lens will cover an energy band from 200-1,300 keV with an effective area reaching 600 cm2. It will be complemented by a…

2009 Experimental Astronomy
INTEGRAL 33
Genetic inversion of sparse disk-integrated photometric data of asteroids: application to Hipparcos data
DOI: 10.1051/0004-6361/200912134 Bibcode: 2009A&A...506..935C

Mottola, S.; Tanga, P.; Cellino, A. +2 more

Context: The development of techniques for the inversion of sparse disk-integrated photometric data of asteroids is a very urgent task, due to the imminent commencements of large sky surveys from both space (Gaia) and the ground (Pan-STARRS).
Aims: We developed a numerical algorithm for the inversion of sparse photometric data of asteroids. An…

2009 Astronomy and Astrophysics
Hipparcos 33
The Sub-Parsec Scale Radio Properties of Southern Starburst Galaxies. II. Supernova Remnants, the Supernova Rate, and the Ionised Medium in the NGC 4945 Starburst
DOI: 10.1088/0004-6256/137/1/537 Bibcode: 2009AJ....137..537L

Tingay, S. J.; Lenc, E.

Wide-field, very long baseline interferometry observations of the nearby starburst galaxy NGC 4945, obtained with the Australian Long Baseline Array, have produced 2.3 GHz images over two epochs with a maximum angular resolution of 15 mas (0.3 pc). Fifteen sources were detected, 13 of which correspond to sources identified in higher frequency (3 c…

2009 The Astronomical Journal
eHST 33
Magnetic helicity accumulation and tilt angle evolution of newly emerging active regions
DOI: 10.1051/0004-6361/200810032 Bibcode: 2009A&A...502..333Y

Zhang, H.; Yang, S.; Büchner, J.

Context: It has been known for years that there is a general dominance of negative (positive) helicity of active regions (ARs) in the northern (southern) solar hemisphere. For a better understanding of the role of helicity in the evolution of active regions, it is necessary to know more about the accumulation of helicity during the emergence of ac…

2009 Astronomy and Astrophysics
SOHO 33
AKARI Detection of Far-Infrared Dust Emission in the Halo of NGC 253
DOI: 10.1088/0004-637X/698/2/L125 Bibcode: 2009ApJ...698L.125K

Onaka, Takashi; Yamagishi, Mitsuyoshi; Kaneda, Hidehiro +1 more

We present new far-infrared (FIR) images of the edge-on starburst galaxy NGC 253 obtained with the Far-Infrared Surveyor (FIS) onboard AKARI at wavelengths of 90 µm and 140 µm. We have clearly detected FIR dust emission extended in the halo of the galaxy; there are two filamentary emission structures extending from the galactic disk up…

2009 The Astrophysical Journal
AKARI 33
A forming disk at z ~ 0.6: collapse of a gaseous disk or major merger remnant?
DOI: 10.1051/0004-6361:200810521 Bibcode: 2009A&A...493..899P

Yang, Y.; Neichel, B.; Flores, H. +2 more

Context: Local spiral galaxies contain roughly two-thirds of the present-day stellar mass density. However, the formation process of disks is still poorly understood.
Aims: We present and analyze observations of J033241.88-274853.9 at z = 0.6679 to understand how its stellar disk was formed.
Methods: We combine multi-wavelength EIS, HST/AC…

2009 Astronomy and Astrophysics
eHST 33
The architecture of the GJ 876 planetary system. Masses and orbital coplanarity for planets b and c
DOI: 10.1051/0004-6361/200811280 Bibcode: 2009A&A...496..249B

Bean, J. L.; Seifahrt, A.

We present a combined analysis of previously published high-precision radial velocities and astrometry for the GJ 876 planetary system using a self-consistent model that accounts for the planet-planet interactions. Assuming the three planets so far identified in the system are coplanar, we find that including the astrometry in the analysis does no…

2009 Astronomy and Astrophysics
eHST 33
Geologic context of in situ rocky exposures in Mare Serpentis, Mars: Implications for crust and regolith evolution in the cratered highlands
DOI: 10.1016/j.icarus.2008.11.026 Bibcode: 2009Icar..200..446R

Rogers, A. D.; Aharonson, O.; Bandfield, J. L.

Global acquisition of infrared spectra and high-resolution visible and infrared imagery has enabled the placement of compositional information within stratigraphic and geologic context. Mare Serpentis, a low albedo region located northwest of Hellas Basin, is rich in spectral and thermophysical diversity and host to numerous isolated exposures of …

2009 Icarus
MEx 32
XMM-Newton observation of the persistent Be/NS X-ray binary pulsar RX J1037.5-5647 in a low luminosity state
DOI: 10.1051/0004-6361/200912538 Bibcode: 2009A&A...505..947L

Tiengo, A.; Mereghetti, S.; Sidoli, L. +2 more

The spectra of several X-ray binary pulsars display a clear soft excess, which in most cases can be described with a blackbody model, above the main power-law component. While in the high-luminosity sources it is usually characterized by low temperature (kT < 0.5 keV) and a large emission radius (R > 100 km), in the two persistent and low-lu…

2009 Astronomy and Astrophysics
XMM-Newton 32