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Evidence for X-ray synchrotron emission from simultaneous mid-IR to X-ray observations of a strong Sgr A* flare

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evidence of a bisymmetric spiral in the Milky Way

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evidence of a thick disk rotation-metallicity correlation

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Evidence of Early Enrichment of the Galactic Disk by Large-Scale Winds

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Evidence of enrichment by individual supernova from elemental abundance ratios in the very metal-poor dSph galaxy Bootes I

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evidence of the inhomogeneity of the stellar population in the differentially reddened globular cluster NGC 3201

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evidence of triggered star formation in G327.3-0.6. Dust-continuum mapping of an infrared dark cloud with P-ArTéMiS

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EVLA Observations of the Barnard 5 Star-Forming Core: Embedded Filaments Revealed

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evolution and lifetime of transient clumps in the turbulent interstellar medium

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evolution of Blister-Type HII Regions in a Magnetized Medium

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Evolution of dust in the Orion Bar with Herschel: I. Radiative transfer modelling

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evolution of Galactic Disks: Multiple Patterns, Radial Migration and Disk Outskirts

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Evolution of growing black holes in axisymmetric galaxy cores

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Evolution of Low- and Intermediate-Mass Stars with [Fe/H] <= -2.5

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evolution of Magnetic Fields and Cosmic Ray Acceleration in Supernova Remnants

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evolution of Super Star Cluster Winds with Strong Cooling

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Evolution of the Barium abundance in the early Galaxy from a NLTE analysis of the Ba lines in a homogeneous sample of EMP stars

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Evolution of the Binary Fraction in Dense Stellar Systems

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Evolution of the binary population in young dense star clusters

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Evolution of the Most Massive Galaxies to z=0.6: I. A New Method for Physical Parameter Estimation

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