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Saturn’s icy satellites investigated by Cassini-VIMS. II. Results at the end of nominal mission
DOI: 10.1016/j.icarus.2009.11.006 Bibcode: 2010Icar..206..507F

Brown, R. H.; Buratti, B. J.; Clark, R. N. +12 more

We report the detailed analysis of the spectrophotometric properties of Saturn's icy satellites as derived by full-disk observations obtained by visual and infrared mapping spectrometer (VIMS) experiment aboard Cassini. In this paper, we have extended the coverage until the end of the Cassini's nominal mission (June 1st 2008), while a previous pap…

2010 Icarus
Cassini 60
Spectroscopic Abundances and Membership in the Wolf 630 Moving Group
DOI: 10.1088/0004-6256/140/2/293 Bibcode: 2010AJ....140..293B

King, Jeremy R.; Bubar, Eric J.

The concept of kinematic assemblages evolving from dispersed stellar clusters has remained contentious since Eggen's initial formulation of moving groups in the 1960s. With high-quality parallaxes from the Hipparcos space astrometry mission, distance measurements for thousands of nearby, seemingly isolated stars are currently available. With these…

2010 The Astronomical Journal
Hipparcos 60
Herschel/HIFI observations of Mars: First detection of O2 at submillimetre wavelengths and upper limits on HCl and H2O2
DOI: 10.1051/0004-6361/201015160 Bibcode: 2010A&A...521L..49H

Blommaert, J. A. D. L.; Küppers, M.; Thomas, N. +47 more

We report on an initial analysis of Herschel/HIFI observations of hydrogen chloride (HCl), hydrogen peroxide (H2O2), and molecular oxygen (O2) in the Martian atmosphere performed on 13 and 16 April 2010 (Ls ~ 77°). We derived a constant volume mixing ratio of 1400 ± 120 ppm for O2 and determin…

2010 Astronomy and Astrophysics
Herschel 60
Chandra Observations of 3C Radio Sources with z < 0.3: Nuclei, Diffuse Emission, Jets, and Hotspots
DOI: 10.1088/0004-637X/714/1/589 Bibcode: 2010ApJ...714..589M

Macchetto, F. D.; Capetti, A.; Gilli, R. +11 more

We report on our Chandra Cycle 9 program to observe half of the 60 (unobserved by Chandra) 3C radio sources at z < 0.3 for 8 ks each. Here we give the basic data: the X-ray intensity of the nuclei and any features associated with radio structures such as hotspots and knots in jets. We have measured fluxes in soft, medium, and hard bands and are…

2010 The Astrophysical Journal
XMM-Newton eHST 60
Extreme flux states of NGC 4151 observed with INTEGRAL
DOI: 10.1111/j.1365-2966.2010.17251.x Bibcode: 2010MNRAS.408.1851L

Paltani, S.; Walter, R.; Ferrigno, C. +5 more

We present a comprehensive spectral analysis of all INTEGRAL data obtained so far for the X-ray-bright Seyfert galaxy NGC 4151. We also use all contemporaneous data from RXTE, XMM-Newton, Swift and Suzaku. We find a linear correlation between the medium- and hard-energy X-ray fluxes measured by INTEGRAL, which indicates an almost constant spectral…

2010 Monthly Notices of the Royal Astronomical Society
INTEGRAL Suzaku XMM-Newton 60
K+a galaxies in the zCOSMOS survey . Physical properties of systems in their post-starburst phase
DOI: 10.1051/0004-6361/200912802 Bibcode: 2010A&A...509A..42V

Bondi, M.; Kneib, J. -P.; Maccagni, D. +60 more


Aims: The identities of the main processes triggering and quenching star-formation in galaxies remain unclear. A key stage in evolution, however, appears to be represented by post-starburst galaxies. To investigate the prevalence of these galaxies and their impact on galaxy evolution in general, we initiated a multiwavelength study of galaxie…

2010 Astronomy and Astrophysics
eHST 60
Panchromatic Observations and Modeling of the HV Tau C Edge-on Disk
DOI: 10.1088/0004-637X/712/1/112 Bibcode: 2010ApJ...712..112D

Pinte, C.; Ménard, F.; Duchêne, G. +12 more

We present new high spatial resolution (lsim0farcs1) 1-5 µm adaptive optics images, interferometric 1.3 mm continuum and 12CO 2-1 maps, and 350 µm, 2.8 and 3.3 mm fluxes measurements of the HV Tau system. Our adaptive optics images unambiguously demonstrate that HV Tau AB-C is a common proper motion pair. They further reveal…

2010 The Astrophysical Journal
eHST 60
NGC 6240: merger-induced star formation and gas dynamics
DOI: 10.1051/0004-6361/201015338 Bibcode: 2010A&A...524A..56E

Genzel, R.; Sturm, E.; Tacconi, L. J. +9 more

We present spatially resolved integral field spectroscopic K-band data at a resolution of 0.13” (60 pc) and interferometric CO(2-1) line observations of the prototypical merging system NGC 6240. Despite the clear rotational signature, the stellar kinematics in the two nuclei are dominated by dispersion. We use Jeans modelling to derive the masses …

2010 Astronomy and Astrophysics
eHST 60
Hard X-ray properties of magnetic cataclysmic variables
DOI: 10.1111/j.1365-2966.2009.15826.x Bibcode: 2010MNRAS.401.2207S

Hill, A. B.; Knigge, C.; Bird, A. J. +10 more

Hard X-ray surveys have proven remarkably efficient in detecting intermediate polars and asynchronous polars, two of the rarest type of cataclysmic variable (CV). Here, we present a global study of hard X-ray-selected intermediate polars and asynchronous polars, focusing particularly on the link between hard X-ray properties and spin/orbital perio…

2010 Monthly Notices of the Royal Astronomical Society
INTEGRAL Suzaku 60
Herschel/HIFI measurements of the ortho/para ratio in water towards Sagittarius B2(M) and W31C
DOI: 10.1051/0004-6361/201015072 Bibcode: 2010A&A...521L..26L

Menten, K. M.; Boulanger, F.; Falgarone, E. +72 more

We present Herschel/HIFI observations of the fundamental rotational transitions of ortho- and para-H_216O and H_218O in absorption towards Sagittarius B2(M) and W31C. The ortho/para ratio in water in the foreground clouds on the line of sight towards these bright continuum sources is generally consistent with the statistical …

2010 Astronomy and Astrophysics
Herschel 60