A search for pre-biotic molecules in hot cores
Journal article, 2007

Aims. Our aim is to better understand the complex chemistry of organic molecules in the interstellar medium, leading to the formation of pre-biotic molecules such as amino acids. Methods. We have performed a search for the pre-biotic molecules amino acetonitrile (H2N CH2 CN) and vinyl acetylene (C2H3 CCH) towards four northern hot core sources using the Onsala 20 m telescope. Results. We have determined upper limits to the column density of amino acetonitrile (1-4*10^13 cm^-2) and vinyl acetylene (2-7*10^14 cm^-2) in the observed sources. In addition, from the absence of other lines within the observed frequency band, we have further constrained the column density of oxiranecarbonitrile (c-C3H3 NO) and amino-ethanol (NH2 CH2 CH2 OH) in these sources.

interstellar molecules

astrobiology

astrochemistry

Author

Eva Wirström

Chalmers, Department of Radio and Space Science, Radio Astronomy and Astrophysics

Per Bergman

Chalmers, Department of Radio and Space Science, National Facility for Radio Astronomy

Åke Hjalmarson

Chalmers, Department of Radio and Space Science, Radio Astronomy and Astrophysics

Albert Nummelin

Chalmers, Computer Science and Engineering (Chalmers)

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 473 177-180

Subject Categories

Astronomy, Astrophysics and Cosmology

More information

Created

10/7/2017