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Gas and dust from the Stars to the Laboratory: Exploring the Nanocosmos
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REACTIVITY OF OH AND CH3OH BETWEEN 22 AND 64 K: MODELING THE GAS PHASE PRODUCTION OF CH3O IN BARNARD 1b

2016/05/20 / Marcelo Castellanos
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Authors: Antinolo, M.; Agundez, M.; Jimenez, E.; Ballesteros, B.; Canosa, A.; El Dib, G.; Albaladejo, J.; Cernicharo, J.

Journal: ASTROPHYSICAL JOURNAL

Publication date: 2016/05/20

DOI: 10.3847/0004-637X/823/1/25

EPMC: PMC4894477

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NANOCOSMOS at the 1st Chilean-Spanish School on Astrochemistry
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Influence of vibration in the reactive scattering of D plus MuH: the effect of dynamical bonding

Nanocosmos has received funding from the European Research Council (ERC) under the European Union´s Seventh Framework Programme (FP7/2007-2013) / ERC-2013-SyG Grant Agreement nº 610256

 

Management contact / web contents:
Dr. Marcelo Castellanos (marcelo.castellanos at csic.es)

Outreach contents:
Natalia Ruiz Zelmanovitch (natalia.r.zelmanovitch at csic.es)

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