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arxiv.org
http://arxiv.org > abs > 1010.3477v3
Cosmic Ray e^+/(e^- + e^+) and pbar/p Ratios Explained by an Injection Model Based on Gamma-ray Observations
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arxiv.org
http://arxiv.org > abs > 1010.2735v1
Free-floating planets: a viable option for panspermia
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arxiv.org
http://arxiv.org > abs > 1010.2727v1
A Multiwavelength Study on the Fate of Ionizing Radiation in Local Starbursts
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arxiv.org
http://arxiv.org > abs > 1010.2490v2
Massive runaway stars in the Small Magellanic Cloud
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arxiv.org
http://arxiv.org > abs > 1010.2093v1
Photochemistry in the inner layers of clumpy circumstellar envelopes: formation of water in C-rich objects and of C-bearing molecules in O-rich objects
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arxiv.org
http://arxiv.org > abs > 1010.2038v3
Reply to 'A Comment on '"The Far Future of Exoplanet Direct Characterization" - the Case for Interstellar Space Probes'
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arxiv.org
http://arxiv.org > abs > 1010.1573v1
A Comment on "The Far Future of Exoplanet Direct Characterization" - the Case for Interstellar Space Probes
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arxiv.org
http://arxiv.org > abs > 1009.5914v1
K 1-6: an asymmetric planetary nebula with a binary central star
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arxiv.org
http://arxiv.org > abs > 1009.5573v4
Study of Interplanetary Magnetic Field with Ground State Alignment
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arxiv.org
http://arxiv.org > abs > 1009.5273v1
Water formation at low temperatures by surface O2 hydrogenation II: the reaction network