Search Publications

The temperature and width of an active fissure on Enceladus measured with Cassini VIMS during the 14 April 2012 South Pole flyover
DOI: 10.1016/j.icarus.2013.07.012 Bibcode: 2013Icar..226.1128G

Hedman, Matthew M.; Sotin, Christophe; Baines, Kevin H. +10 more

The width and temperature of the active fissures on Saturn’s satellite Enceladus provide key observable constraints on physical models of these geyser-like eruptions. We analyze a sequence of high spatial resolution near-infrared spectra acquired with VIMS at 0.025 s intervals during a 74 km altitude flyover of the South Pole of Enceladus by the C…

2013 Icarus
Cassini 70
The ACS LCID Project. IX. Imprints of the Early Universe in the Radial Variation of the Star Formation History of Dwarf Galaxies
DOI: 10.1088/0004-637X/778/2/103 Bibcode: 2013ApJ...778..103H

Skillman, Evan D.; Dolphin, Andrew; Monelli, Matteo +8 more

Based on Hubble Space Telescope observations from the Local Cosmology from Isolated Dwarfs project, we present the star formation histories, as a function of galactocentric radius, of four isolated Local Group dwarf galaxies: two dSph galaxies, Cetus and Tucana, and two transition galaxies (dTrs), LGS-3 and Phoenix. The oldest stellar populations …

2013 The Astrophysical Journal
eHST 70
On the self-regulation of intense star-formation in galaxies at z = 1-3
DOI: 10.1051/0004-6361/201220555 Bibcode: 2013A&A...555A..72L

Boulanger, F.; Lehnert, M. D.; Di Matteo, P. +3 more

We have analyzed the properties of the Hα and [Nii]λ6583 rest-frame optical emission lines of a sample of 53 intensely star forming galaxies at z = 1.3 to 2.7 observed with SINFONI on the ESO-VLT. Similar to previous authors, we find large velocity dispersions in the lines, σ = few 10-250 km s-1. Our data agree well with simulations whe…

2013 Astronomy and Astrophysics
eHST 70
Long-term variation in the cloud-tracked zonal velocities at the cloud top of Venus deduced from Venus Express VMC images
DOI: 10.1029/2011JE004013 Bibcode: 2013JGRE..118...37K

Futaana, Yoshifumi; Imamura, Takeshi; Kouyama, Toru +2 more

We present observational evidence of the variation of the cloud-tracked zonal velocity by ~20 m s-1 with a timescale of a few hundred days in the southern low latitude region based on an analysis of cloud images taken by the Venus Monitoring Camera on board Venus Express. A spectral analysis suggests that the variation has a periodicity…

2013 Journal of Geophysical Research (Planets)
VenusExpress 70
Properties of a Solar Flare Kernel Observed by Hinode and SDO
DOI: 10.1088/0004-637X/766/2/127 Bibcode: 2013ApJ...766..127Y

Young, P. R.; Doschek, G. A.; Warren, H. P. +1 more

Flare kernels are compact features located in the solar chromosphere that are the sites of rapid heating and plasma upflow during the rise phase of flares. An example is presented from a M1.1 class flare in active region AR 11158 observed on 2011 February 16 07:44 UT for which the location of the upflow region seen by EUV Imaging Spectrometer (EIS…

2013 The Astrophysical Journal
Hinode 70
Optical constants of refractory oxides at high temperatures. Mid-infrared properties of corundum, spinel, and α-quartz, potential carriers of the 13 µm feature
DOI: 10.1051/0004-6361/201220459 Bibcode: 2013A&A...553A..81Z

Mutschke, H.; Zeidler, S.; Posch, Th.

Context. Many cosmic dust species, among them refractory oxides, form at temperatures higher than 300 K. Nevertheless, most astrophysical studies are based on the room-temperature optical constants of solids, such as corundum and spinel. A more realistic approach is needed for these materials, especially in the context of modeling late-type stars.…

2013 Astronomy and Astrophysics
ISO 70
Kinematics of massive star ejecta in the Milky Way as traced by 26Al
DOI: 10.1051/0004-6361/201322563 Bibcode: 2013A&A...559A..99K

Wang, Wei; Gerhard, Ortwin; Diehl, Roland +5 more

Context. Massive stars form in groups and their winds and supernova explosions create superbubbles up to kpc in size. The fate of their ejecta is of vital importance for the dynamics of the interstellar medium, for chemical evolution models, and the chemical enrichment of galactic halos and the intergalactic medium. However, ejecta kinematics and …

2013 Astronomy and Astrophysics
INTEGRAL 70
Data-based modelling of the Earth's dynamic magnetosphere: a review
DOI: 10.5194/angeo-31-1745-2013 Bibcode: 2013AnGeo..31.1745T

Tsyganenko, N. A.

This paper reviews the main advances in the area of data-based modelling of the Earth's distant magnetic field achieved during the last two decades. The essence and the principal goal of the approach is to extract maximum information from available data, using physically realistic and flexible mathematical structures, parameterized by the most rel…

2013 Annales Geophysicae
Cluster 70
The shape of broad-line profiles in active galactic nuclei
DOI: 10.1051/0004-6361/201219411 Bibcode: 2013A&A...549A.100K

Kollatschny, W.; Zetzl, M.


Aims: We present a study of the broad optical/UV emission line profiles in active galactic nuclei (AGN) to get information on the dominant velocity components (turbulence, rotation, etc.) in the central broad-line region (BLR).
Methods: We introduce line broadening simulations of emission line profiles and compare these results with the …

2013 Astronomy and Astrophysics
eHST 70
An Exponential Decline at the Bright End of the z = 6 Galaxy Luminosity Function
DOI: 10.1088/0004-6256/145/1/4 Bibcode: 2013AJ....145....4W

Willott, Chris J.; Kneib, Jean-Paul; Ilbert, Olivier +7 more

We present the results of a search for the most luminous star-forming galaxies at redshifts z ≈ 6 based on Canada-France-Hawaii Telescope Legacy Survey data. We identify a sample of 40 Lyman break galaxies (LBGs) brighter than magnitude z' = 25.3 across an area of almost 4 deg2. Sensitive spectroscopic observations of seven galaxies pro…

2013 The Astronomical Journal
eHST 70