The Open UniversitySkip to content
 

A hot core laboratory

van Broekhuizen, Fleur A.; Fraser, Helen J.; Schutte, Willem A.; de Kuijper, Ewie and van Dishoeck, Ewine F. (2002). A hot core laboratory. In: conference proceedings pp. 434–436.

Warning

This is the latest version of this eprint.

URL: http://adsabs.harvard.edu/abs/2003cdsf.conf..434V
Google Scholar: Look up in Google Scholar

Abstract

The newly-built Cryogenic Photoproduct Analysis Device (CRYOPAD) will simulate Hot Core chemistry in the laboratory. Hot Cores (HC's) represent the most chemically rich areas of the insterstellar medium. They are characterised as warm (100-200K), dense (n_H_2 = 10cm-3) regions, that are in most cases associated with high mass star formation. Internal heating and ultraviolet radiation that may be present inside HC's cause processing and evaporation of ice mantles around infalling grains. This initiates a rich chemistry among the gaseous molecules that leads to the formation of a wide range of complex organics. Gas-phase chemistry models are however not always able to explain the observed molecular abundances. Therefore surface chemistry and solid state chemistry probably contribute to the production of complex organics as well.

CRYOPAD is an experimental setup that is specifically designed to study the solid state chemistry of interstellar ice analogs by radiative and thermal processing. Ultra High Vacuum conditions (8x10-11mbar) will minimize contamination of the sample, which is essential for the analysis of trace products of the processing. The gas analysis is performed in situ by a Quadrupole Mass Spectrometer. Additionally CRYOPAD has the option of looking at the surface chemistry by Reflective Absorption Infrared Spectrometry in the 4000-400 cm-1 region.

The research will focus on the production of small volatile complex organics such as simple esters and ethers like methyl formate and dimethyl ether. The results will be used to interpret the observational data of HC's in further detail and to perform a directed search for molecules in space with only weak observable features. Furthermore the laboratory data will be used to refine chemical models of HC's. Thus we hope to gain a better understanding of the physical and chemical processes associated with high mass star formation.

Item Type: Conference or Workshop Item
Copyright Holders: 2002 Not known
Extra Information: Chemistry as a Diagnostic of Star Formation
Proceedings of the Conference held in Waterloo, Canada, August 21-23, 2002
Edited by Charles L. Curry, Michel Fich
ISBN: 978-0-660-19089-1
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Related URLs:
Item ID: 37320
Depositing User: Stephen Serjeant
Date Deposited: 24 Jun 2013 09:52
Last Modified: 19 Dec 2017 10:04
URI: http://oro.open.ac.uk/id/eprint/37320
Share this page:

Available Versions of this Item

  • A hot core laboratory. (deposited 24 Jun 2013 09:52) [Currently Displayed]

Actions (login may be required)

Policies | Disclaimer

© The Open University   contact the OU