Search for HOOH in Orion⋆⋆⋆

Author： Liseau R.   Larsson B.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|583|issue|A53-A53

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.583, Iss.issue, 2015-10, pp. : A53-A53

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

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Abstract

Context. The abundance of key molecules determines the level of cooling that is necessary for the formation of stars and planetary systems. In this context, one needs to understand the details of the time dependent oxygen chemistry, leading to the formation of O2 and H2O.

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