Search Publications

Observational Evidence for High Neutronization in Supernova Remnants: Implications for Type Ia Supernova Progenitors
DOI: 10.3847/1538-4357/aa72f8 Bibcode: 2017ApJ...843...35M

Mori, Hideyuki; Yamaguchi, Hiroya; Badenes, Carles +8 more

The physical process whereby a carbon-oxygen white dwarf explodes as a Type Ia supernova (SN Ia) remains highly uncertain. The degree of neutronization in SN Ia ejecta holds clues to this process because it depends on the mass and the metallicity of the stellar progenitor, and on the thermodynamic history prior to the explosion. We report on a new…

2017 The Astrophysical Journal
Suzaku 39
Magnetic reconnection during eruptive magnetic flux ropes
DOI: 10.1051/0004-6361/201731146 Bibcode: 2017A&A...604L...7M

Lin, J.; Roussev, I. I.; Keppens, R. +1 more


Aims: We perform a three-dimensional (3D) high resolution numerical simulation in isothermal magnetohydrodynamics to study the magnetic reconnection process in a current sheet (CS) formed during an eruption of a twisted magnetic flux rope (MFR). Because the twist distribution violates the Kruskal-Shafranov condition, the kink instability occu…

2017 Astronomy and Astrophysics
SOHO 39
Gas Sloshing Regulates and Records the Evolution of the Fornax Cluster
DOI: 10.3847/1538-4357/aa989e Bibcode: 2017ApJ...851...69S

Jones, Christine; Nulsen, Paul E. J.; Kraft, Ralph P. +7 more

We present results of a joint Chandra and XMM-Newton analysis of the Fornax Cluster, the nearest galaxy cluster in the southern sky. Signatures of merger-induced gas sloshing can be seen in the X-ray image. We identify four sloshing cold fronts in the intracluster medium, residing at radii of 3 kpc (west), 10 kpc (northeast), 30 kpc (southwest), a…

2017 The Astrophysical Journal
XMM-Newton 39
Dust Abundance Variations in the Magellanic Clouds: Probing the Life-cycle of Metals with All-sky Surveys
DOI: 10.3847/1538-4357/aa7067 Bibcode: 2017ApJ...841...72R

Bot, Caroline; Roman-Duval, Julia; Gordon, Karl +1 more

Observations and modeling suggest that dust abundance (gas-to-dust ratio, G/D) depends on (surface) density. Variations of the G/D provide timescale constraints for the different processes involved in the life cycle of metals in galaxies. Recent G/D measurements based on Herschel data suggest a factor of 5-10 decrease in dust abundance between the…

2017 The Astrophysical Journal
Planck 39
The HDUV Survey: Six Lyman Continuum Emitter Candidates at z ∼ 2 Revealed by HST UV Imaging
DOI: 10.3847/1538-4357/aa8863 Bibcode: 2017ApJ...847...12N

Oesch, P. A.; Carollo, C. M.; Nelson, E. J. +14 more

We present six galaxies at z∼ 2 that show evidence of Lyman continuum (LyC) emission based on the newly acquired UV imaging of the Hubble Deep UV legacy survey (HDUV) conducted with the WFC3/UVIS camera on the Hubble Space Telescope (HST). At the redshift of these sources, the HDUV F275W images partially probe the ionizing continuum. By exploiting…

2017 The Astrophysical Journal
eHST 39
Disruption of Saturn's quasi-periodic equatorial oscillation by the great northern storm
DOI: 10.1038/s41550-017-0271-5 Bibcode: 2017NatAs...1..765F

Fletcher, Leigh N.; Irwin, Patrick G. J.; Flasar, F. Michael +7 more

The equatorial middle atmospheres of the Earth1, Jupiter2 and Saturn3,4 all exhibit a remarkably similar phenomenon—a vertical, cyclic pattern of alternating temperatures and zonal (east-west) wind regimes that propagate slowly downwards with a well-defined multi-year period. Earth's quasi-biennial oscillation (QBO…

2017 Nature Astronomy
Cassini 39
Galactic winds with MUSE: A direct detection of Fe II* emission from a z = 1.29 galaxy
DOI: 10.1051/0004-6361/201730428 Bibcode: 2017A&A...605A.118F

Bacon, Roland; Finley, Hayley; Bouché, Nicolas +13 more

Emission signatures from galactic winds provide an opportunity to directly map the outflowing gas, but this is traditionally challenging because of the low surface brightness. Using very deep observations (27 h) of the Hubble Deep Field South with the Multi Unit Spectroscopic Explorer (MUSE) instrument, we identify signatures of an outflow in both…

2017 Astronomy and Astrophysics
eHST 38
Staying away from the bar: the local dynamical signature of slow and fast bars in the Milky Way
DOI: 10.1093/mnras/stw2807 Bibcode: 2017MNRAS.465.1443M

Siebert, Arnaud; Famaey, Benoit; Bienaymé, Olivier +3 more

Both the three-dimensional density of red clump giants and the gas kinematics in the inner Galaxy indicate that the pattern speed of the Galactic bar could be much lower than previously estimated. Here, we show that such slow bar models are unable to reproduce the bimodality observed in local stellar velocity space. We do so by computing the respo…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 38
Formation of Methylamine and Ethylamine in Extraterrestrial Ices and Their Role as Fundamental Building Blocks of Proteinogenic α-amino Acids
DOI: 10.3847/1538-4357/aa7edd Bibcode: 2017ApJ...845...83F

Kaiser, Ralf I.; Förstel, Marko; Bergantini, Alexandre +2 more

The -CH-NH2 moiety represents the fundamental building block of all proteinogenic amino acids, with the cyclic amino acid proline being a special case (-CH-NH- in proline). Exploiting a chemical retrosynthesis, we reveal that methylamine (CH3NH2) and/or ethylamine (CH3CH2NH2) are es…

2017 The Astrophysical Journal
Rosetta 38
Powerful outflows in the central parsecs of the low-luminosity active galactic nucleus NGC 1386
DOI: 10.1093/mnras/stx1401 Bibcode: 2017MNRAS.470.2845R

Prieto, M. A.; Luque, R.; Müller-Sánchez, F. +3 more

Low-luminosity active galactic nuclei, I.e. L_{bol}/Ledd ∼ 10-6-10-3, constitute the bulk population of active galactic nuclei (AGNs). Powerful jets, common in these objects, are a crucial source of feedback energy-driving mass outflows into the host galaxy and the intergalactic medium. This paper reports the first…

2017 Monthly Notices of the Royal Astronomical Society
eHST 38