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arxiv.org
http://arxiv.org > abs > 1703.03119v3
Tracing magnetic fields with spectroscopic channel maps
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arxiv.org
http://arxiv.org > abs > 1703.02043v1
Spatial structure of several diffuse interstellar band carriers
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arxiv.org
http://arxiv.org > abs > 1703.00504v2
Strong HI Lyman-$α$ variations from the 11 Gyr-old host star Kepler-444: a planetary origin ?
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arxiv.org
http://arxiv.org > abs > 1702.08729v2
$\mathit{Chempy}$: A flexible chemical evolution model for abundance fitting - Do the Sun's abundances alone constrain chemical evolution models?
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arxiv.org
http://arxiv.org > abs > 1702.08456v1
Estimating Extinction using Unsupervised Machine Learning
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arxiv.org
http://arxiv.org > abs > 1702.02546v4
Decaying Fermionic Dark Matter Search with CALET
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arxiv.org
http://arxiv.org > abs > 1702.01001v1
Cosmic-Ray Anisotropy and the Local Interstellar Turbulence
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arxiv.org
http://arxiv.org > abs > 1701.08618v2
Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries
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arxiv.org
http://arxiv.org > abs > 1701.06585v1
The PAH emission characteristics of the reflection nebula NGC2023
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arxiv.org
http://arxiv.org > abs > 1701.06409v1
The Possibility of Forming Propargyl Alcohol in the Interstellar Medium