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Favicon of arxiv.org
arxiv.org
http://arxiv.org > abs > 1411.0009v2
Modelling the supernova-driven ISM in different environments
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arxiv.org
http://arxiv.org > abs > 1410.8531v1
Shell-Shocked: The Interstellar Medium Near Cygnus X-1
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arxiv.org
http://arxiv.org > abs > 1410.8247v1
The second epoch Molonglo Galactic Plane Survey: images and candidate supernova remnants
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arxiv.org
http://arxiv.org > abs > 1410.8190v1
Detection of a Light Echo from the Otherwise Normal SN 2007af
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arxiv.org
http://arxiv.org > abs > 1410.8161v1
Star formation quenching in simulated group and cluster galaxies: When, how, and why?
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arxiv.org
http://arxiv.org > abs > 1410.8136v2
Searching for Inflationary B-modes: Can dust emission properties be extrapolated from 350 GHz to 150 GHz?
Favicon of arxiv.org
arxiv.org
http://arxiv.org > abs > 1410.8092v2
Rossby wave instability does not require sharp resistivity gradients
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arxiv.org
http://arxiv.org > abs > 1410.7938v1
Propagation of cosmic rays into diffuse clouds
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arxiv.org
http://arxiv.org > abs > 1410.7861v1
Evolution of grain size distribution in high-redshift dusty quasars: Integrating large amounts of dust and unusual extinction curves
Favicon of arxiv.org
arxiv.org
http://arxiv.org > abs > 1410.7840v1
Can Cosmic Rays Interacting With Molecular Clouds Explain The Galactic Center Gamma-Ray Excess?