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Very Deep inside the SN 1987A Core Ejecta: Molecular Structures Seen in 3D
DOI: 10.3847/2041-8213/aa784c Bibcode: 2017ApJ...842L..24A

van Loon, J. Th.; Larsson, J.; Lundqvist, P. +21 more

Most massive stars end their lives in core-collapse supernova explosions and enrich the interstellar medium with explosively nucleosynthesized elements. Following core collapse, the explosion is subject to instabilities as the shock propagates outward through the progenitor star. Observations of the composition and structure of the innermost regio…

2017 The Astrophysical Journal
eHST 46
CHEERS: The chemical evolution RGS sample
DOI: 10.1051/0004-6361/201629926 Bibcode: 2017A&A...607A..98D

Zhang, Y. -Y.; Finoguenov, A.; Böhringer, H. +17 more

Context. The chemical yields of supernovae and the metal enrichment of the intra-cluster medium (ICM) are not well understood. The hot gas in clusters of galaxies has been enriched with metals originating from billions of supernovae and provides a fair sample of large-scale metal enrichment in the Universe. High-resolution X-ray spectra of cluster…

2017 Astronomy and Astrophysics
XMM-Newton 45
Magnetized Kelvin-Helmholtz instability: theory and simulations in the Earth's magnetosphere context
DOI: 10.1017/S0022377817000770 Bibcode: 2017JPlPh..83f5301F

Califano, Francesco; Faganello, Matteo

The Kelvin-Helmholtz instability, proposed a long time ago for its role in and impact on the transport properties at magnetospheric flanks, has been widely investigated in the Earth's magnetosphere context. This review covers more than fifty years of theoretical and numerical efforts in investigating the evolution of Kelvin-Helmholtz vortices and …

2017 Journal of Plasma Physics
Cluster 45
Constraints on Quenching of Z ≲ 2 Massive Galaxies from the Evolution of the Average Sizes of Star-forming and Quenched Populations in COSMOS
DOI: 10.3847/1538-4357/aa697a Bibcode: 2017ApJ...839...71F

Ilbert, O.; Scoville, N. Z.; Carollo, C. M. +5 more

We use >9400 {log}(m/{M})> 10 quiescent and star-forming galaxies at z ≲ 2 in COSMOS/UltraVISTA to study the average size evolution of these systems, with focus on the rare ultra-massive population at {log}(m/{M})> 11.4. The large 2 square degree survey area delivers a sample of ∼400 such ultra-massive systems. A…

2017 The Astrophysical Journal
eHST 45
WASP-167b/KELT-13b: joint discovery of a hot Jupiter transiting a rapidly rotating F1V star
DOI: 10.1093/mnras/stx1729 Bibcode: 2017MNRAS.471.2743T

Queloz, D.; Ségransan, D.; Collier Cameron, A. +46 more

We report the joint WASP/KELT discovery of WASP-167b/KELT-13b, a transiting hot Jupiter with a 2.02-d orbit around a V = 10.5, F1V star with [Fe/H] = 0.1 ± 0.1. The 1.5 RJup planet was confirmed by Doppler tomography of the stellar line profiles during transit. We place a limit of <8 MJup on its mass. The planet is in a re…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 45
Hot oxygen escape from Mars: Simple scaling with solar EUV irradiance
DOI: 10.1002/2016JA023461 Bibcode: 2017JGRA..122.1102C

Luhmann, J.; Cravens, T. E.; Combi, M. +8 more

The evolution of the atmosphere of Mars and the loss of volatiles over the lifetime of the solar system is a key topic in planetary science. An important loss process for atomic species, such as oxygen, is ionospheric photochemical escape. Dissociative recombination of O2+ ions (the major ion species) produces fast oxygen ato…

2017 Journal of Geophysical Research (Space Physics)
MEx 45
Resolved astrometric orbits of ten O-type binaries
DOI: 10.1051/0004-6361/201629260 Bibcode: 2017A&A...601A..34L

Absil, O.; Ertel, S.; Grellmann, R. +11 more


Aims: Our long-term aim is to derive model-independent stellar masses and distances for long period massive binaries by combining apparent astrometric orbit with double-lined radial velocity amplitudes (SB2).
Methods: We followed-up ten O+O binaries with AMBER, PIONIER and GRAVITY at the VLTI. Here, we report on 130 astrometric observati…

2017 Astronomy and Astrophysics
Gaia 45
Deuteration of ammonia in the starless core Ophiuchus/H-MM1
DOI: 10.1051/0004-6361/201628463 Bibcode: 2017A&A...600A..61H

Daniel, F.; Schlemmer, S.; Güsten, R. +13 more

Context. Ammonia and its deuterated isotopologues probe physical conditions in dense molecular cloud cores. The time-dependence of deuterium fractionation and the relative abundances of different nuclear spin modifications are supposed to provide a means of determining the evolutionary stages of these objects.
Aims: We aim to test the current…

2017 Astronomy and Astrophysics
Herschel 45
Lyman continuum leaking AGN in the SSA22 field
DOI: 10.1093/mnras/stw1329 Bibcode: 2017MNRAS.465..302M

Inoue, Akio K.; Iwata, Ikuru; Micheva, Genoveva

Subaru/SuprimeCam narrow-band photometry of the SSA22 field reveals the presence of four Lyman continuum (LyC) candidates among a sample of 14 active galactic nuclei (AGNs). Two show offsets and likely have stellar LyCin nature or are foreground contaminants. The remaining two LyC candidates are type I AGN. We argue that the average LyC escape fra…

2017 Monthly Notices of the Royal Astronomical Society
eHST 45
Morpho-kinematics of z ∼ 1 galaxies probe the hierarchical scenario
DOI: 10.1093/mnras/stw2711 Bibcode: 2017MNRAS.465.1157R

Flores, H.; Hammer, F.; Puech, M. +2 more

We have studied a representative sample of intermediate-mass galaxies at z ∼ 1, observed by the kinematic survey KMOS3D. We have re-estimated the kinematical parameters from the published kinematic maps and analysed photometric data from Hubble Space Telescope (HST) to measure optical disc inclinations and Position Angle. We find that o…

2017 Monthly Notices of the Royal Astronomical Society
eHST 45