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arxiv.org
http://arxiv.org > abs > 1411.5858v1
Heteroatom-doped hydrogenated amorphous carbons, a-C:H:X 'Volatile' silicon, sulphur and nitrogen depletion, blue photoluminescence, diffuse interstellar bands and ferro-magnetic carbon grain connections (Research Note)
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arxiv.org
http://arxiv.org > abs > 1411.5854v1
A framework for resolving the origin, nature and evolution of the diffuse interstellar band carriers?
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arxiv.org
http://arxiv.org > abs > 1411.5513v1
On the origin of the faint-end of the red sequence in high density environments
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arxiv.org
http://arxiv.org > abs > 1411.5402v1
3D Dust Mapping Reveals that Orion Forms Part of a Large Ring of Dust
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arxiv.org
http://arxiv.org > abs > 1411.5373v1
An accurate and efficient algorithm for detection of radio bursts with an unknown dispersion measure, for single dish telescopes and interferometers
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arxiv.org
http://arxiv.org > abs > 1411.5264v1
Tidal Downsizing model. I. Numerical methods: saving giant planets from tidal disruptions
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arxiv.org
http://arxiv.org > abs > 1411.5055v1
HD/H2 as a probe of the roles of gas, dust, light, metallicity and cosmic rays in promoting the growth of molecular hydrogen in the diffuse interstellar medium
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arxiv.org
http://arxiv.org > abs > 1411.5027v2
Probing the Physical Conditions of Atomic Gas at High Redshift
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arxiv.org
http://arxiv.org > abs > 1411.5017v1
XMM-Newton Measurement of the Galactic Halo X-ray Emission using a Compact Shadowing Cloud
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arxiv.org
http://arxiv.org > abs > 1411.5013v2
Carriers of 4964 and 6196 diffuse interstellar bands and environments dominated by either CH or CH$^{+}$ molecules