Search Publications

Shape, topography, gravity anomalies and tidal deformation of Titan
DOI: 10.1016/j.icarus.2014.03.018 Bibcode: 2014Icar..236..169M

Lunine, Jonathan I.; Hayes, Alex; Zebker, Howard +5 more

Gravity measurements and elevation data from the Cassini mission have been used to create shape, global topography and gravity anomaly models of Titan that enable an improved understanding of its outer ice I shell structure. We provide constraints on the averaged ice shell thickness and its long-wavelength lateral variations, as well as the densit…

2014 Icarus
Cassini 83
The distribution of interstellar dust in CALIFA edge-on galaxies via oligochromatic radiative transfer fitting
DOI: 10.1093/mnras/stu612 Bibcode: 2014MNRAS.441..869D

De Looze, Ilse; Baes, Maarten; Fritz, Jacopo +5 more

We investigate the amount and spatial distribution of interstellar dust in edge-on spiral galaxies, using detailed radiative transfer modelling of a homogeneous sample of 12 galaxies selected from the Calar Alto Legacy Integral Field Area survey. Our automated fitting routine, FITSKIRT, was first validated against artificial data. This is done by …

2014 Monthly Notices of the Royal Astronomical Society
Herschel 82
Dust and gas in luminous proto-cluster galaxies at z = 4.05: the case for different cosmic dust evolution in normal and starburst galaxies
DOI: 10.1051/0004-6361/201423905 Bibcode: 2014A&A...569A..98T

Daddi, E.; Elbaz, D.; Béthermin, M. +14 more

We measure the dust and gas content of the three submillimeter galaxies (SMGs) in the GN20 proto-cluster at z = 4.05 using new IRAM Plateau de Bure interferometer (PdBI) CO(4-3) and 1.2-3.3 mm continuum observations. All these three SMGs are heavily dust obscured, with UV-based star formation rate (SFR) estimates significantly smaller than the one…

2014 Astronomy and Astrophysics
eHST 82
A hidden reservoir of Fe/FeS in interstellar silicates?
DOI: 10.1051/0004-6361/201423985 Bibcode: 2014A&A...565L...9K

Ysard, N.; Jones, A.; Köhler, M.

Context. The depletion of iron and sulphur into dust in the interstellar medium and the exact nature of interstellar amorphous silicate grains is still an open question.
Aims: We study the incorporation of iron and sulphur into amorphous silicates of olivine- and pyroxene-types and their effects on the dust spectroscopy and thermal emission. …

2014 Astronomy and Astrophysics
ISO 82
Infall of Nearby Galaxies into the Virgo Cluster as Traced with Hubble Space Telescope
DOI: 10.1088/0004-637X/782/1/4 Bibcode: 2014ApJ...782....4K

Dolphin, Andrew E.; Wu, Po-Feng; Shaya, Edward J. +2 more

We measured the tip of the red giant branch distances to nine galaxies in the direction to the Virgo cluster using the Advanced Camera for Surveys on the Hubble Space Telescope. These distances put seven galaxies (GR 34, UGC 7512, NGC 4517, IC 3583, NGC 4600, VCC 2037, and KDG 215) in front of Virgo and two galaxies (IC 3023 and KDG 177) likely in…

2014 The Astrophysical Journal
eHST 82
Standard Rulers, Candles, and Clocks from the Low-Redshift Universe
DOI: 10.1103/PhysRevLett.113.241302 Bibcode: 2014PhRvL.113x1302H

Verde, Licia; Jimenez, Raul; Heavens, Alan

We measure the length of the baryon acoustic oscillation (BAO) feature, and the expansion rate of the recent Universe, from low-redshift data only, almost model independently. We make only the following minimal assumptions: homogeneity and isotropy, a metric theory of gravity, a smooth expansion history, and the existence of standard candles (supe…

2014 Physical Review Letters
Planck 82
Far-Infrared Surveys of Galaxy Evolution
DOI: 10.1146/annurev-astro-081913-035953 Bibcode: 2014ARA&A..52..373L

Lutz, Dieter

Roughly half of the radiation from evolving galaxies in the early Universe reaches us in the far-infrared and submillimeter wavelength ranges. Recent major advances in observing capabilities, in particular the launch of the Herschel Space Observatory in 2009, have dramatically enhanced our ability to use this information in the context of multiwav…

2014 Annual Review of Astronomy and Astrophysics
Herschel 82
Molecular Gas in the X-Ray Bright Group NGC 5044 as Revealed by ALMA
DOI: 10.1088/0004-637X/792/2/94 Bibcode: 2014ApJ...792...94D

Ohyama, Youichi; Brighenti, Fabrizio; Jones, Christine +17 more

An ALMA observation of the early-type galaxy NGC 5044, which resides at the center of an X-ray bright group with a moderate cooling flow, detected 24 molecular structures within the central 2.5 kpc. The masses of the molecular structures vary from 3 × 105 M to 107 M and the CO(2-1) linewidths vary fr…

2014 The Astrophysical Journal
eHST 81
Warm Breeze from the Starboard Bow: a New Population of Neutral Helium in the Heliosphere
DOI: 10.1088/0067-0049/213/2/29 Bibcode: 2014ApJS..213...29K

Wurz, P.; McComas, D. J.; Fuselier, S. A. +9 more

We investigate the signals from neutral helium atoms observed in situ from Earth orbit in 2010 by the Interstellar Boundary Explorer (IBEX). The full helium signal observed during the 2010 observation season can be explained as a superposition of pristine neutral interstellar He gas and an additional population of neutral helium that we call the W…

2014 The Astrophysical Journal Supplement Series
Ulysses 81
Herschel Multitiered Extragalactic Survey: clusters of dusty galaxies uncovered by Herschel and Planck
DOI: 10.1093/mnras/stt2253 Bibcode: 2014MNRAS.439.1193C

Pérez-Fournon, I.; Clements, D. L.; de Zotti, G. +21 more

The potential for Planck to detect clusters of dusty, star-forming galaxies at z > 1 is tested by examining the Herschel-SPIRE images of Planck Early Release Compact Source Catalog sources lying in fields observed by the Herschel Multitiered Extragalactic Survey. Of the 16 Planck sources that lie in the ∼90 sq. deg. examined, we find that 12 ar…

2014 Monthly Notices of the Royal Astronomical Society
Herschel Planck 81