The early stages of star formation: glycolaldehyde and its isomers as dense core tracers
Lead Research Organisation:
University College London
Department Name: Physics and Astronomy
Abstract
We have been awarded (and scheduled over 4 nights) 16 hours of observing time at the JCMT in Hawaii, for project M13AU21. We are proposing to observe the simple sugar glycolaldehyde and its isomers in order to understand the physical and chemical conditions in hot molecular cores, sites of massive star formation. Our team previously found glycolaldehyde to be more compact than any other molecule in G31.41+0.31, thereby tracing the densest, hottest inner region of this hot core. Its isomers may also trace these inner regions, allowing us to further probe the conditions at the very centre of the core. Understanding the abundance ratio of these isomers can constrain hot core chemistry and reveal physical conditions and chemical pathways. We are requesting travel and subsistence money for Hannah Calcutt to go observing at the JCMT (note that we have been scheduled in 1 month time and we have only been told few days ago about it).
Organisations
People |
ORCID iD |
Serena Viti (Principal Investigator) |
Publications
Bell T
(2014)
Extended warm gas in Orion KL as probed by methyl cyanide
in Astronomy & Astrophysics
Burke D
(2015)
Glycolaldehyde, methyl formate and acetic acid adsorption and thermal desorption from interstellar ices
in Monthly Notices of the Royal Astronomical Society
Burke DJ
(2015)
Trapping and desorption of complex organic molecules in water at 20 K.
in The Journal of chemical physics
Jiménez-Serra I
(2014)
DETECTABILITY OF GLYCINE IN SOLAR-TYPE SYSTEM PRECURSORS
in The Astrophysical Journal
Occhiogrosso A
(2014)
Ethylene oxide and acetaldehyde in hot cores
in Astronomy & Astrophysics
Description | We observed 3 isomers of an important pre-biotic molecule in space |
Exploitation Route | We now need to observe the same isomers in a larger sample of objects |
Sectors | Other |