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Orbits and Photometry of Pluto's Satellites: Charon, S/2005 P1, and S/2005 P2
DOI: 10.1086/504422 Bibcode: 2006AJ....132..290B

Stern, S. Alan; Young, Leslie A.; Buie, Marc W. +2 more

We present new astrometry of Pluto's three satellites from images taken of the Pluto system during 2002-2003 with the High Resolution Camera mode of the Advanced Camera for Surveys instrument on the Hubble Space Telescope. The observations were designed to produce an albedo map of Pluto, but they also contain images of Charon and the two recently …

2006 The Astronomical Journal
eHST 85
Mid-Infrared Spectroscopy of Carbon Stars in the Small Magellanic Cloud
DOI: 10.1086/504516 Bibcode: 2006ApJ...645.1118S

Price, S. D.; Wood, P. R.; Matsuura, M. +3 more

We have observed a sample of 36 objects in the Small Magellanic Cloud (SMC) with the Infrared Spectrometer on the Spitzer Space Telescope. Nineteen of these sources are carbon stars. An examination of the near- and mid-infrared photometry shows that the carbon-rich and oxygen-rich dust sources follow two easily separated sequences. A comparison of…

2006 The Astrophysical Journal
ISO 84
Titan Radar Mapper observations from Cassini's T3 fly-by
DOI: 10.1038/nature04786 Bibcode: 2006Natur.441..709E

Stiles, B.; Kelleher, K.; Callahan, P. +32 more

Cassini's Titan Radar Mapper imaged the surface of Saturn's moon Titan on its February 2005 fly-by (denoted T3), collecting high-resolution synthetic-aperture radar and larger-scale radiometry and scatterometry data. These data provide the first definitive identification of impact craters on the surface of Titan, networks of fluvial cha…

2006 Nature
Cassini 84
First observation of Mars with XMM-Newton. High resolution X-ray spectroscopy with RGS
DOI: 10.1051/0004-6361:20054253 Bibcode: 2006A&A...451..709D

Holmström, M.; Gunell, H.; Burwitz, V. +7 more

In the first observation of Mars with XMM-Newton, on 20-21 November 2003, this planet is clearly detected as an X-ray source. High resolution X-ray spectroscopy with the Reflection Grating Spectrometer (RGS) confirms that the X-ray radiation from Mars is composed of two different components: one due to fluorescent scattering of solar X-rays in its…

2006 Astronomy and Astrophysics
XMM-Newton 84
A FUSE Survey of High-Latitude Galactic Molecular Hydrogen
DOI: 10.1086/500365 Bibcode: 2006ApJS..163..282W

Wakker, B. P.

Measurements of molecular hydrogen (H2) column densities are presented for the first six rotational levels (J=0-5) for 73 extragalactic targets observed with the Far Ultraviolet Spectroscopic Explorer (FUSE). All of these have a final signal-to-noise ratio larger than 10 and are located at Galactic latitude |b|>20deg. The …

2006 The Astrophysical Journal Supplement Series
eHST 83
The broad-band spectrum of Cygnus X-1 measured by INTEGRAL
DOI: 10.1051/0004-6361:20053068 Bibcode: 2006A&A...446..591C

Goldoni, P.; Rodriguez, J.; Foschini, L. +9 more

The INTEGRAL satellite extensively observed the black hole binary Cygnus X-1 from 2002 November to 2004 November during calibration, open time and core program (Galactic Plane Scan) observations. These data provide evidence for significant spectral variations over the period. In the framework of the accreting black hole phenomenology, the source w…

2006 Astronomy and Astrophysics
INTEGRAL 83
Unveiling the nature of INTEGRAL objects through optical spectroscopy. III. Observations of seven southern sources
DOI: 10.1051/0004-6361:20054332 Bibcode: 2006A&A...449.1139M

Palazzi, E.; Masetti, N.; Charles, P. A. +9 more

Context: . The detection, thanks to the INTEGRAL satellite, of a number of new hard X-ray sources calls for the identification of their nature by means of observations at longer wavelengths. Aims. In our continuing campaign to identify longer-wavelength counterparts of these newly-discovered hard X-ray sources detected by INTEGRAL, we observed the…

2006 Astronomy and Astrophysics
INTEGRAL 83
Self-gravity wakes in Saturn's A ring measured by stellar occultations from Cassini
DOI: 10.1029/2005GL025163 Bibcode: 2006GeoRL..33.7201C

Sremčević, M.; Colwell, J. E.; Esposito, L. W.

An azimuthal brightness asymmetry in Saturn's A ring is caused by ephemeral agglomerations that continually form under the mutual gravity of the ring particles only to be torn apart by Keplerian shear. We calculate the shape and spacing of the self-gravity wakes from Cassini stellar occultations. The wakes are highly flatttened structures, with he…

2006 Geophysical Research Letters
Cassini 83
The vertical structure of Titan's upper atmosphere from Cassini Ion Neutral Mass Spectrometer measurements
DOI: 10.1016/j.icarus.2005.10.029 Bibcode: 2006Icar..182..567Y

Waite, J. H.; Kasprzak, W. T.; Müller-Wodarg, I. +4 more

Data acquired by the Ion Neutral Mass Spectrometer (INMS) on the Cassini spacecraft during its close encounter with Titan on 26 October 2004 reveal the structure of its upper atmosphere. Altitude profiles of N 2, CH 4, and H 2, inferred from INMS measurements, determine the temperature, vertical mixing rate, and es…

2006 Icarus
Cassini 83
Discovery of Ultracompact Dwarf Galaxies in the Virgo Cluster
DOI: 10.1086/497960 Bibcode: 2006AJ....131..312J

Drinkwater, M. J.; Jones, J. B.; Phillipps, S. +7 more

We have discovered nine ultracompact dwarf galaxies (UCDs) in the Virgo Cluster, extending samples of these objects outside the Fornax Cluster. Using the Two Degree Field (2dF) multifiber spectrograph on the Anglo-Australian Telescope, the new Virgo members were found among 1500 color-selected, starlike targets with 16.0<bj<20.2 i…

2006 The Astronomical Journal
eHST 82