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Favicon of arxiv.org
arxiv.org
http://arxiv.org > abs > 1410.6573v1
On the viability of the PAH model as an explanation of the unidentified infrared emission features
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arxiv.org
http://arxiv.org > abs > 1410.6428v1
Star formation around the mid-infrared bubble CN 148
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arxiv.org
http://arxiv.org > abs > 1410.6343v1
Pore evolution in interstellar ice analogues: simulating the effects of temperature increase
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arxiv.org
http://arxiv.org > abs > 1410.7432v1
Optical Multi-Channel Intensity Interferometry - or: How To Resolve O-Stars in the Magellanic Clouds
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arxiv.org
http://arxiv.org > abs > 1410.6092v1
Polytropic models of filamentary interstellar clouds -II. Helical magnetic fields
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arxiv.org
http://arxiv.org > abs > 1410.6091v1
Polytropic models of filamentary interstellar clouds - I. Structure and stability
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arxiv.org
http://arxiv.org > abs > 1410.5889v1
The dynamics of collapsing cores and star formation
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arxiv.org
http://arxiv.org > abs > 1410.5709v6
The influence of supernova remnants on the interstellar medium in the Large Magellanic Cloud seen at 20--600 $μ$m wavelengths
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arxiv.org
http://arxiv.org > abs > 1410.5433v1
Ejection of globular cluster interstellar media through ionization by white dwarfs
Favicon of arxiv.org
arxiv.org
http://arxiv.org > abs > 1410.5669v1
Hyperfine excitation of N$_2$H$^+$ by H$_2$: Toward a revision of N$_2$H$^+$ abundance in cold molecular clouds