Search Publications

Solar Wind Interaction and Impact on the Venus Atmosphere
DOI: 10.1007/s11214-017-0362-8 Bibcode: 2017SSRv..212.1453F

Barabash, Stas; Stenberg Wieser, Gabriella; Futaana, Yoshifumi +1 more

Venus has intrigued planetary scientists for decades because of its huge contrasts to Earth, in spite of its nickname of "Earth's Twin". Its invisible upper atmosphere and space environment are also part of the larger story of Venus and its evolution. In 60s to 70s, several missions (Venera and Mariner series) explored Venus-solar wind interaction…

2017 Space Science Reviews
VenusExpress 92
Coupling hydrodynamics with comoving frame radiative transfer. I. A unified approach for OB and WR stars
DOI: 10.1051/0004-6361/201730642 Bibcode: 2017A&A...603A..86S

Hamann, W. -R.; Sander, A. A. C.; Shenar, T. +2 more

Context. For more than two decades, stellar atmosphere codes have been used to derive the stellar and wind parameters of massive stars. Although they have become a powerful tool and sufficiently reproduce the observed spectral appearance, they can hardly be used for more than measuring parameters. One major obstacle is their inconsistency between …

2017 Astronomy and Astrophysics
IUE 92
The Chandra COSMOS Legacy Survey: Energy Spectrum of the Cosmic X-Ray Background and Constraints on Undetected Populations
DOI: 10.3847/1538-4357/aa5ea4 Bibcode: 2017ApJ...837...19C

Treister, E.; Comastri, Andrea; Elvis, Martin +15 more

Using Chandra observations in the 2.15 deg2 COSMOS-legacy field, we present one of the most accurate measurements of the Cosmic X-ray Background (CXB) spectrum to date in the [0.3-7] keV energy band. The CXB has three distinct components: contributions from two Galactic collisional thermal plasmas at kT ∼ 0.27 and 0.07 keV and an extrag…

2017 The Astrophysical Journal
INTEGRAL 92
High Lyman Continuum Escape Fraction in a Lensed Young Compact Dwarf Galaxy at z = 2.5
DOI: 10.3847/2041-8213/aa5ff7 Bibcode: 2017ApJ...837L..12B

Fan, Xiaohui; Jiang, Linhua; Cai, Zheng +2 more

We present the HST WFC3/F275W UV imaging observations of A2218-Flanking, a lensed compact dwarf galaxy at redshift z≈ 2.5. The stellar mass of A2218-Flanking is {log}({M}* /{M})={9.14}-0.04+0.07 and SFR is {12.5}-7.4+3.8 {M} yr-1 after correcting the magnif…

2017 The Astrophysical Journal
eHST 91
Lensing substructure quantification in RXJ1131-1231: a 2 keV lower bound on dark matter thermal relic mass
DOI: 10.1088/1475-7516/2017/05/037 Bibcode: 2017JCAP...05..037B

Amara, Adam; Refregier, Alexandre; Birrer, Simon

We study the substructure content of the strong gravitational lens RXJ1131-1231 through a forward modelling approach that relies on generating an extensive suite of realistic simulations. We use a semi-analytic merger tree prescription that allows us to stochastically generate substructure populations whose properties depend on the dark matter par…

2017 Journal of Cosmology and Astroparticle Physics
eHST 91
A representative survey of the dynamics and energetics of FR II radio galaxies
DOI: 10.1093/mnras/stx189 Bibcode: 2017MNRAS.467.1586I

Hardcastle, M. J.; Croston, J. H.; Ineson, J. +1 more

We report the first large, systematic study of the dynamics and energetics of a representative sample of Fanaroff-Riley type II (FR II) radio galaxies with well-characterized group/cluster environments. We used X-ray inverse-Compton and radio synchrotron measurements to determine the internal radio-lobe conditions, and these were compared with ext…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 91
The Origins of [C II] Emission in Local Star-forming Galaxies
DOI: 10.3847/1538-4357/aa8035 Bibcode: 2017ApJ...845...96C

Boquien, M.; Rigopoulou, D.; Armus, L. +17 more

The [C II] 158 µm fine-structure line is the brightest emission line observed in local star-forming galaxies. As a major coolant of the gas-phase interstellar medium, [C II] balances the heating, including that due to far-ultraviolet photons, which heat the gas via the photoelectric effect. However, the origin of [C II] emission remains uncl…

2017 The Astrophysical Journal
Herschel 91
A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 Microns
DOI: 10.3847/1538-4365/aa6476 Bibcode: 2017ApJS..230....1L

Gao, Yu; Díaz-Santos, Tanio; Lu, Nanyao +18 more

We describe a Herschel Space Observatory 194-671 µm spectroscopic survey of a sample of 121 local luminous infrared galaxies and report the fluxes of the CO J to J-1 rotational transitions for 4≤slant J≤slant 13, the [N II] 205 µm line, the [C I] lines at 609 and 370 µm, as well as additional and usually fainter lines. The CO spe…

2017 The Astrophysical Journal Supplement Series
Herschel 91
The Complete Infrared View of Active Galactic Nuclei from the 70 Month Swift/BAT Catalog
DOI: 10.3847/1538-4357/835/1/74 Bibcode: 2017ApJ...835...74I

Ueda, Yoshihiro; Kawamuro, Taiki; Ricci, Claudio +5 more

We systematically investigate the near- to far-infrared (FIR) photometric properties of a nearly complete sample of local active galactic nuclei (AGNs) detected in the Swift/Burst Alert Telescope (BAT) all-sky ultra-hard X-ray (14-195 keV) survey. Out of 606 non-blazar AGNs in the Swift/BAT 70 month catalog at high galactic latitudes of | b| > …

2017 The Astrophysical Journal
AKARI Herschel 91
ATLASGAL-selected massive clumps in the inner Galaxy. III. Dust continuum characterization of an evolutionary sample
DOI: 10.1051/0004-6361/201526841 Bibcode: 2017A&A...599A.139K

König, C.; Menten, K. M.; Csengeri, T. +8 more

Context. Massive-star formation and the processes involved are still poorly understood. The ATLASGAL survey provides an ideal basis for detailed studies of large numbers of massive-star forming clumps covering the whole range of evolutionary stages. The ATLASGAL Top100 is a sample of clumps selected by their infrared and radio properties to be rep…

2017 Astronomy and Astrophysics
Herschel 91