Search Publications

The stratigraphy of the Amenthes region, Mars: Time limits for the formation of fluvial, volcanic and tectonic landforms
DOI: 10.1016/j.icarus.2011.06.041 Bibcode: 2011Icar..215..128E

Hiesinger, H.; Ivanov, M. A.; Erkeling, G. +2 more

We present results of our morphologic and stratigraphic investigations in the Amenthes region for which our observations suggest a complex spatial and temporal interrelation between volcanic and possibly water-related processes. We have produced a series of self-consistent geological maps and a stratigraphic correlation chart that show the spatial…

2011 Icarus
MEx 16
The high-velocity cloud complex Galactic center negative as seen by EBHIS and GASS. I. Cloud catalog and global properties
DOI: 10.1051/0004-6361/201117357 Bibcode: 2011A&A...533A.105W

Kerp, J.; Winkel, B.; Flöer, L. +3 more

Using Milky Way data of the new Effelsberg-Bonn H i Survey (EBHIS) and the Galactic All-Sky Survey (GASS), we present a revised picture of the high-velocity cloud (HVC) complex Galactic center negative (GCN). Owing to the higher angular resolution of these surveys compared to previous studies (e.g., the Leiden Dwingeloo Survey), we resolve complex…

2011 Astronomy and Astrophysics
eHST 16
First VLBI Detection of the Radio Remnant of Supernova 1987A: Evidence for Small-scale Features
DOI: 10.1088/2041-8205/728/1/L15 Bibcode: 2011ApJ...728L..15N

Gaensler, B. M.; Ng, C. -Y.; Staveley-Smith, L. +5 more

We present a detailed analysis of the first very long baseline interferometry (VLBI) detection of the radio remnant of supernova 1987A. The VLBI data taken in 2007 and 2008 at 1.4 and 1.7 GHz, respectively, provide images sensitive to angular scales from 0farcs1 to 0farcs7, the highest resolution to date at radio frequencies. The results reveal tw…

2011 The Astrophysical Journal
eHST 16
Results from the 2009 campaign on WR 140
Bibcode: 2011BSRSL..80..595W

Williams, Peredur

The archetypal Wolf-Rayet + O star colliding-wind binary WR 140 has a very elliptical orbit, so that maximum interaction between the WR and O winds, and the most rapid changes in configuration, occur around periastron passage. To exploit this laboratory for studying wind-collision and high-energy phenomena, several groups mounted campaigns to obse…

2011 Bulletin de la Societe Royale des Sciences de Liege
XMM-Newton 16
On the stability of clathrate hydrates in comets 67P/Churyumov-Gerasimenko and 46P/Wirtanen
DOI: 10.1051/0004-6361/201015438 Bibcode: 2011A&A...525A.144M

Weaver, H. A.; Mousis, O.; Schmitt, B. +3 more

Context. For several years, Jupiter-family comets have been the targets of spacecraft missions whose aims are to determine the comets' composition, structure, and physical properties. The Rosetta mission is currently flying towards comet 67P/Churyumov Gerasimenko for a rendezvous in August 2014 and comet 46P/Wirtanen is considered for a rendezvous…

2011 Astronomy and Astrophysics
Rosetta 16
The Mass-Radius Relation for Star-forming Galaxies at z ~ 1.5-3.0
DOI: 10.1088/2041-8205/735/1/L19 Bibcode: 2011ApJ...735L..19N

Shapley, Alice E.; Steidel, Charles C.; Law, David R. +1 more

We present early results from a Hubble Space Telescope WFC3/IR imaging survey of star-forming galaxies in the redshift range 1.5 < z < 3.0. When complete, this survey will consist of 42 orbits of F160W imaging distributed amongst 10 survey fields on the line of sight to bright background QSOs, covering 65 arcmin2 to a depth of 27.…

2011 The Astrophysical Journal
eHST 16
AKARI Near-infrared Spectral Observations of Shocked H2 Gas of the Supernova Remnant IC 443
DOI: 10.1088/0004-637X/732/2/124 Bibcode: 2011ApJ...732..124S

Koo, Bon-Chul; Lee, Ho-Gyu; Seon, Kwang-Il +1 more

We present near-infrared (2.5-5.0 µm) spectra of shocked H2 gas in the supernova remnant IC 443, obtained with the satellite AKARI. Three shocked clumps—known as B, C, and G—and one background region were observed, and only H2 emission lines were detected. Except in clump B, the extinction-corrected level population sho…

2011 The Astrophysical Journal
AKARI ISO 16
A galaxy as the source of a C IV absorption system close to the epoch of reionization
DOI: 10.1111/j.1365-2966.2011.19534.x Bibcode: 2011MNRAS.418..820D

Pettini, Max; Madau, Piero; Díaz, C. Gonzalo +2 more

We find a bright (LUV= 2.5 Lz= 6) Lyα emitter (LAE) at redshift z= 5.719 at a projected distance of 79 physical kpc from a strong triply ionized carbon (C IV) absorption system at redshift z= 5.7238 previously reported in the spectrum of the zem= 6.309 quasi-stellar object SDSS J1030+0524. This is the h…

2011 Monthly Notices of the Royal Astronomical Society
eHST 16
Studying methane and other trace species in the Mars atmosphere using a SOIR instrument
DOI: 10.1016/j.pss.2010.05.009 Bibcode: 2011P&SS...59..292D

Daerden, F.; Robert, S.; Neary, L. +7 more

Solar Occultation in the InfraRed (SOIR) is one of three spectrometers of the SPICAV/SOIR instrument suite ( Bertaux et al., 2007b) on board the Venus Express orbiter (VEX). VEX has been in orbit around Venus since April 2006 and to date SOIR has carried out over 674 measurements. Pre-launch and in-orbit performance analyses allow us to predict wh…

2011 Planetary and Space Science
VenusExpress 16
High-Resolution Optical and Near-Infrared Images of the FS Tauri Circumbinary Disk
DOI: 10.1093/pasj/63.3.543 Bibcode: 2011PASJ...63..543H

Hayashi, Masahiko; Fukagawa, Misato; Itoh, Yoichi +2 more

We present an H-band image of FS Tauri, a 0.''2-separated classical T Tauri binary system, taken with the Coronagraphic Imager with Adaptive Optics (CIAO) on the Subaru Telescope. This new image, combined with Hubble Space Telescope/Advanced Camera for Surveys (HST/ACS) F606W-band polarimetric images, shows that the binary has complicated circumbi…

2011 Publications of the Astronomical Society of Japan
eHST 16