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Xenon isotopes in 67P/Churyumov-Gerasimenko show that comets contributed to Earth's atmosphere
DOI: 10.1126/science.aal3496 Bibcode: 2017Sci...356.1069M

Wurz, P.; Altwegg, K.; Balsiger, H. +27 more

The origin of cometary matter and the potential contribution of comets to inner-planet atmospheres are long-standing problems. During a series of dedicated low-altitude orbits, the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) on the Rosetta spacecraft analyzed the isotopes of xenon in the coma of comet 67P/Churyumov-Gerasimen…

2017 Science
Rosetta 160
The Stellar Initial Mass Function in Early-type Galaxies from Absorption Line Spectroscopy. III. Radial Gradients
DOI: 10.3847/1538-4357/aa7135 Bibcode: 2017ApJ...841...68V

van Dokkum, Pieter; Romanowsky, Aaron J.; Conroy, Charlie +2 more

There is good evidence that the centers of massive early-type galaxies have a bottom-heavy stellar initial mass function (IMF) compared to that of the Milky Way. Here we study the radial variation of the IMF within such galaxies, using a combination of high-quality Keck spectroscopy and a new suite of stellar population synthesis models that cover…

2017 The Astrophysical Journal
eHST 160
On the generation of solar spicules and Alfvénic waves
DOI: 10.1126/science.aah5412 Bibcode: 2017Sci...356.1269M

De Pontieu, B.; Martínez-Sykora, J.; Hansteen, V. H. +3 more

In the lower solar atmosphere, the chromosphere is permeated by jets known as spicules, in which plasma is propelled at speeds of 50 to 150 kilometers per second into the corona. The origin of the spicules is poorly understood, although they are expected to play a role in heating the million-degree corona and are associated with Alfvénic waves tha…

2017 Science
IRIS 158
Powering prolonged hydrothermal activity inside Enceladus
DOI: 10.1038/s41550-017-0289-8 Bibcode: 2017NatAs...1..841C

Postberg, Frank; Sotin, Christophe; Čadek, Ondřej +4 more

Geophysical data from the Cassini spacecraft imply the presence of a global ocean underneath the ice shell of Enceladus1, only a few kilometres below the surface in the South Polar Terrain2-4. Chemical analyses indicate that the ocean is salty5 and is fed by ongoing hydrothermal activity6-8. In order to …

2017 Nature Astronomy
Cassini 158
Geoeffective Properties of Solar Transients and Stream Interaction Regions
DOI: 10.1007/s11214-017-0411-3 Bibcode: 2017SSRv..212.1271K

Balogh, A.; Kilpua, E. K. J.; von Steiger, R. +1 more

Interplanetary Coronal Mass Ejections (ICMEs), their possible shocks and sheaths, and co-rotating interaction regions (CIRs) are the primary large-scale heliospheric structures driving geospace disturbances at the Earth. CIRs are followed by a faster stream where Alfvénic fluctuations may drive prolonged high-latitude activity. In this paper we hi…

2017 Space Science Reviews
Ulysses 157
Paving the way for the JWST: witnessing globular cluster formation at z > 3
DOI: 10.1093/mnras/stx351 Bibcode: 2017MNRAS.467.4304V

Castellano, M.; Pentericci, L.; Grillo, C. +17 more

We report on five compact, extremely young (<10 Myr) and blue (βUV < -2.5, Fλ = λβ) objects observed with VLT/Multi Unit Spectroscopic Explorer at redshifts 3.1169 and 3.235, in addition to three objects at z = 6.145. These sources are strongly magnified (3-40 times) by the Hubble Frontier Field galaxy cluste…

2017 Monthly Notices of the Royal Astronomical Society
eHST 157
Comoving Stars in Gaia DR1: An Abundance of Very Wide Separation Comoving Pairs
DOI: 10.3847/1538-3881/aa6ffd Bibcode: 2017AJ....153..257O

Hogg, David W.; Morton, Timothy D.; Price-Whelan, Adrian M. +2 more

The primary sample of the Gaia Data Release 1 is the Tycho-Gaia Astrometric Solution (TGAS): ≈2 million Tycho-2 sources with improved parallaxes and proper motions relative to the initial catalog. This increased astrometric precision presents an opportunity to find new binary stars and moving groups. We search for high-confidence comoving pairs of…

2017 The Astronomical Journal
Gaia 157
Machine-learned Identification of RR Lyrae Stars from Sparse, Multi-band Data: The PS1 Sample
DOI: 10.3847/1538-3881/aa661b Bibcode: 2017AJ....153..204S

Grebel, Eva K.; Magnier, Eugene A.; Rix, Hans-Walter +16 more

RR Lyrae stars may be the best practical tracers of Galactic halo (sub-)structure and kinematics. The PanSTARRS1 (PS1) 3π survey offers multi-band, multi-epoch, precise photometry across much of the sky, but a robust identification of RR Lyrae stars in this data set poses a challenge, given PS1's sparse, asynchronous multi-band light curves (≲ 12 …

2017 The Astronomical Journal
Gaia 157
Evidence for the formation of comet 67P/Churyumov-Gerasimenko through gravitational collapse of a bound clump of pebbles
DOI: 10.1093/mnras/stx2741 Bibcode: 2017MNRAS.469S.755B

Shi, Xian; Blum, Jürgen; Della Corte, Vincenzo +19 more

The processes that led to the formation of the planetary bodies in the Solar system are still not fully understood. Using the results obtained with the comprehensive suite of instruments onboard the European Space Agency's Rosetta mission, we present evidence that comet 67P/Churyumov-Gerasimenko likely formed through the gentle gravitational colla…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 156
The California-Kepler Survey. II. Precise Physical Properties of 2025 Kepler Planets and Their Host Stars
DOI: 10.3847/1538-3881/aa80e7 Bibcode: 2017AJ....154..108J

Cargile, Phillip A.; Morton, Timothy D.; Fulton, Benjamin J. +11 more

We present stellar and planetary properties for 1305 Kepler Objects of Interest hosting 2025 planet candidates observed as part of the California-Kepler Survey. We combine spectroscopic constraints, presented in Paper I, with stellar interior modeling to estimate stellar masses, radii, and ages. Stellar radii are typically constrained to 11%, comp…

2017 The Astronomical Journal
Gaia 156