Search Publications

Possible temperate lakes on Titan
DOI: 10.1016/j.icarus.2015.05.009 Bibcode: 2015Icar..257..313V

Sotin, Christophe; Barnes, Jason W.; Le Mouélic, Stéphane +5 more

We analyze southern mid-latitude albedo-dark features on Titan observed by Cassini's Visual and Infrared Mapping Spectrometer (VIMS). In exploring the nature of these features we consider their morphology, albedo, and specular reflectivity. We suggest that they represent candidates for potential temperate lakes. The presence of lakes at the mid-la…

2015 Icarus
Cassini 14
The Megasecond Chandra X-Ray Visionary Project Observation of NGC 3115. II. Properties of Point Sources
DOI: 10.1088/0004-637X/808/1/19 Bibcode: 2015ApJ...808...19L

Romanowsky, Aaron J.; Brodie, Jean P.; Remillard, Ronald A. +7 more

We carried out an in-depth study of low-mass X-ray binaries (LMXBs) detected in the nearby lenticular galaxy NGC 3115 using the Megasecond Chandra X-ray Visionary Project observation (total exposure time 1.1 Ms). In total we found 136 candidate LMXBs in the field and 49 in globular clusters (GCs) above 2σ detection, with 0.3-8 keV luminosity L

2015 The Astrophysical Journal
eHST 14
First Taste of Hot Channel in Interplanetary Space
DOI: 10.1088/0004-637X/803/2/96 Bibcode: 2015ApJ...803...96S

Chen, Y.; Song, H. Q.; Cheng, X. +3 more

A hot channel (HC) is a high temperature (∼10 MK) structure in the inner corona first revealed by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory. Eruptions of HCs are often associated with flares and coronal mass ejections (CMEs). Results of previous studies have suggested that an HC is a good proxy for a magnetic flux ro…

2015 The Astrophysical Journal
SOHO 14
High pressure Cavity Ring Down Spectroscopy: Application to the absorption continuum of CO2 near 1.7 µm
DOI: 10.1016/j.jqsrt.2015.08.014 Bibcode: 2015JQSRT.167...97K

Campargue, A.; Tran, H.; Mondelain, D. +1 more

A Cavity Ring Down Spectrometer has been developed for high sensitivity absorption spectroscopy in the near infrared at pressure up to 10 bar. In order to strictly avoid perturbations of the optical alignment by pressure forces, the pre-aligned CRDS cavity is inserted inside the high pressure cell. The stability of the spectra baseline has been va…

2015 Journal of Quantitative Spectroscopy and Radiative Transfer
VenusExpress 14
Predicting the CIB-φ contamination in the cross-correlation of the tSZ effect and φ
DOI: 10.1051/0004-6361/201525714 Bibcode: 2015A&A...575L..11H

Hurier, G.

The recent release of Planck data gives access to a full sky coverage of the thermal Sunyaev-Zel'dovich (tSZ) effect and of the cosmic microwave background (CMB) lensing potential (φ). The cross-correlation of these two probes of the large-scale structures in the Universe is a powerful tool for testing cosmological models, especially in the contex…

2015 Astronomy and Astrophysics
Planck 14
NGC 4370: a case study for testing our ability to infer dust distribution and mass in nearby galaxies
DOI: 10.1051/0004-6361/201526147 Bibcode: 2015A&A...579A.103V

Ferrarese, L.; Boquien, M.; Bianchi, S. +14 more

Context. A segment of the early-type galaxy population hosts a prominent dust lane, often decoupled from its stellar body. Methods of quantifying the dust content of these systems based on optical imaging data usually yield dust masses that are an order of magnitude lower than dust masses derived from the observed far-IR (FIR) emission. The discre…

2015 Astronomy and Astrophysics
Herschel 14
Multiwavelength modeling the SED of supersoft X-ray sources. II. RS Ophiuchi: From the explosion to the SSS phase
DOI: 10.1016/j.newast.2013.12.005 Bibcode: 2015NewA...36..128S

Skopal, A.

RS Oph is a recurrent symbiotic nova that undergoes nova-like outbursts on a time scale of 20 yr. Its two last eruptions (1985 and 2006) were subject of intensive multiwavelengths observational campaign from the X-rays to the radio. This contribution aims to determine physical parameters and the ionization structure of the nova from its explosion …

2015 New Astronomy
IUE XMM-Newton 14
Pursuing the Planet-Debris Disk Connection: Analysis of Upper Limits from the Anglo-Australian Planet Search
DOI: 10.1088/0004-6256/149/2/86 Bibcode: 2015AJ....149...86W

Wittenmyer, Robert A.; Marshall, Jonathan P.

Solid material in protoplanetary disks will suffer one of two fates after the epoch of planet formation; either being bound up into planetary bodies, or remaining in smaller planetesimals to be ground into dust. These end states are identified through detection of sub-stellar companions by periodic radial velocity (or transit) variations of the st…

2015 The Astronomical Journal
Herschel 14
COSIMA-Rosetta calibration for in situ characterization of 67P/Churyumov-Gerasimenko cometary inorganic compounds
DOI: 10.1016/j.pss.2015.05.005 Bibcode: 2015P&SS..117...35K

Trieloff, Mario; Krüger, Harald; Fischer, Henning +15 more

COmetary Secondary Ion Mass Analyzer (COSIMA) is a time-of-flight secondary ion mass spectrometry (TOF-SIMS) instrument on board the Rosetta space mission. COSIMA has been designed to measure the composition of cometary dust particles. It has a mass resolution m/Δm of 1400 at mass 100 u, thus enabling the discrimination of inorganic mass peaks fro…

2015 Planetary and Space Science
Rosetta 14
Cepheid Variables in the Maser-host Galaxy NGC 4258
DOI: 10.1088/0004-6256/149/6/183 Bibcode: 2015AJ....149..183H

Macri, Lucas M.; Hoffmann, Samantha L.

We present results of a ground-based survey for Cepheid variables in NGC 4258. This galaxy plays a key role in the Extragalactic Distance Scale due to its very precise and accurate distance determination via very long baseline interferometry observations of water masers. We imaged two fields within this galaxy using the Gemini North telescope and …

2015 The Astronomical Journal
eHST 14