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Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields
DOI: 10.1007/s11214-017-0354-8 Bibcode: 2017SSRv..212..193P

Wurz, P.; Fichtner, H.; Scherer, K. +11 more

This paper summarizes the results obtained by the team "Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields" supported by the International Space Science Institute (ISSI) in Bern, Switzerland. We focus on the physical processes occurring in the outer heliosphere, especially at i…

2017 Space Science Reviews
Ulysses VenusExpress 70
Surface changes on comet 67P/Churyumov-Gerasimenko suggest a more active past
DOI: 10.1126/science.aak9384 Bibcode: 2017Sci...355.1392E

Jorda, L.; Lara, L. M.; Bertaux, J. -L. +53 more

The Rosetta spacecraft spent ~2 years orbiting comet 67P/Churyumov-Gerasimenko, most of it at distances that allowed surface characterization and monitoring at submeter scales. From December 2014 to June 2016, numerous localized changes were observed, which we attribute to cometary-specific weathering, erosion, and transient events driven by expos…

2017 Science
Rosetta 70
Fundamental Physics with the Hubble Frontier Fields: Constraining Dark Matter Models with the Abundance of Extremely Faint and Distant Galaxies
DOI: 10.3847/1538-4357/836/1/61 Bibcode: 2017ApJ...836...61M

Castellano, M.; Grazian, A.; Menci, N. +4 more

We show that the measured abundance of ultra-faint lensed galaxies at z≈ 6 in the Hubble Frontier Fields (HFF) provides stringent constraints on the parameter space of (I) dark matter models based on keV sterile neutrinos; (II) “fuzzy” wavelike dark matter models, based on Bose-Einstein condensates of ultra-light particles. For the case of sterile…

2017 The Astrophysical Journal
eHST 70
The MUSE Hubble Ultra Deep Field Survey. V. Spatially resolved stellar kinematics of galaxies at redshift 0.2 ≲ z ≲ 0.8
DOI: 10.1051/0004-6361/201730905 Bibcode: 2017A&A...608A...5G

Bacon, Roland; Bouché, Nicolas; Contini, Thierry +11 more

We present spatially resolved stellar kinematic maps, for the first time, for a sample of 17 intermediate redshift galaxies (0.2 ≲ z ≲ 0.8). We used deep MUSE/VLT integral field spectroscopic observations in the Hubble Deep Field South (HDFS) and Hubble Ultra Deep Field (HUDF), resulting from ≈30 h integration time per field, each covering 1' × 1'…

2017 Astronomy and Astrophysics
eHST 70
Discovery of a low-mass companion inside the debris ring surrounding the F5V star HD 206893
DOI: 10.1051/0004-6361/201629908 Bibcode: 2017A&A...597L...2M

Pinte, C.; Dent, W. R. F.; del Burgo, C. +30 more


Aims: Uncovering the ingredients and the architecture of planetary systems is a very active field of research that has fuelled many new theories on giant planet formation, migration, composition, and interaction with the circumstellar environment. We aim at discovering and studying new such systems, to further expand our knowledge of how low-…

2017 Astronomy and Astrophysics
eHST 70
Gaia 1 and 2. A pair of new Galactic star clusters
DOI: 10.1093/mnras/stx1182 Bibcode: 2017MNRAS.470.2702K

Belokurov, V.; Koposov, Sergey E.; Torrealba, G.

We present the results of the very first search for faint Milky Way satellites in the Gaia data. Using stellar positions only, we are able to re-discover objects detected in much deeper data as recently as the last couple of years. While we do not identify new prominent ultrafaint dwarf galaxies, we report the discovery of two new star clusters, G…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 69
The Global Solar Dynamo
DOI: 10.1007/s11214-015-0230-3 Bibcode: 2017SSRv..210..367C

Cameron, R. H.; Dikpati, M.; Brandenburg, A.

A brief summary of the various observations and constraints that underlie solar dynamo research are presented. The arguments that indicate that the solar dynamo is an alpha-omega dynamo of the Babcock-Leighton type are then shortly reviewed. The main open questions that remain are concerned with the subsurface dynamics, including why sunspots emer…

2017 Space Science Reviews
Ulysses 69
ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z 2 using [CI] and CO
DOI: 10.1051/0004-6361/201730391 Bibcode: 2017A&A...602A..11P

van Dokkum, Pieter G.; Nelson, Erica J.; De Breuck, Carlos +9 more

We present ALMA detections of the [CI] 1-0, CO J = 3-2, and CO J = 4-3 emission lines, as well as the ALMA band 4 continuum for a compact star-forming galaxy (cSFG) at z = 2.225, 3D-HST GS30274. As is typical for cSFGs, this galaxy has a stellar mass of 1.89 ± 0.47 × 1011M, with a star formation rate (SFR) of 214 ± 44 M

2017 Astronomy and Astrophysics
eHST 69
Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
DOI: 10.1088/1475-7516/2017/05/040 Bibcode: 2017JCAP...05..040G

Zhang, Jing-Fei; Zhang, Xin; Li, Yun-He +1 more

We constrain the neutrino mass in the scenario of vacuum energy interacting with cold dark matter by using current cosmological observations. To avoid the large-scale instability problem in interacting dark energy models, we employ the parameterized post-Friedmann (PPF) approach to do the calculation of perturbation evolution, for the Q = βHρ

2017 Journal of Cosmology and Astroparticle Physics
Planck 69
Internal delensing of Planck CMB temperature and polarization
DOI: 10.1088/1475-7516/2017/05/035 Bibcode: 2017JCAP...05..035C

Challinor, Anthony; Carron, Julien; Lewis, Antony

We present a first internal delensing of CMB maps, both in temperature and polarization, using the public foreground-cleaned (SMICA) Planck 2015 maps. After forming quadratic estimates of the lensing potential, we use the corresponding displacement field to undo the lensing on the same data. We build differences of the delensed spectra to the orig…

2017 Journal of Cosmology and Astroparticle Physics
Planck 69