The 12C/13C ratio in the galactic center: Implications for galactic chemical evolution and isotope chemistry

Halfen, DeWayne T.

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https://hdl.handle.net/2142/97020 Copy

Description

Title

The 12C/13C ratio in the galactic center: Implications for galactic chemical evolution and isotope chemistry

Author(s)

Halfen, DeWayne T.

Contributor(s)

Ziurys, Lucy M.

Issue Date

2017-06-20

Keyword(s)

Astronomy

Abstract

Observations from a spectral-line survey of Sgr B2(N) of the $^{12}$C and $^{13}$C isotopologues of H$_2$CS, CH$_3$CCH, NH$_2$CHO, CH$_2$CHCN, and CH$_3$CH$_2$CN have been analyzed to more accurately establish the $^{12}$C/$^{13}$C ratio in this cloud. The wide spectral coverage has enabled an accurate evaluation of the $^{12}$C/$^{13}$C ratios in these low abundance molecules, based on numerous transitions. The lines typically exhibited two distinct velocity components at 64 and 73 km s$^{-1}$. The $^{12}$C/$^{13}$C ratio was found to be in the range 18-24 for all 5 molecules, for optically thin transitions, with an average value of 20.5, and did not significantly vary between the two velocity components. The Galactic gradient has been revised to be $^{12}$C/$^{13}$C = 6.08(0.48) $D_{GC}$ + 15.7(2.9). Furthermore, the $^{12}$C/$^{13}$C ratio did not change with substitution site on the molecule. Therefore, there appears to be very little chemical fractionation or isotope-selective photodissociation occurring in Sgr B2(N), and the $^{12}$C/$^{13}$C ratios are a true reflection of the isotopic abundances generated by stellar nucleosynthesis.

Publisher

International Symposium on Molecular Spectroscopy

Type of Resource

text

Language

eng

Permalink

http://hdl.handle.net/2142/97020

DOI

https://doi.org/10.15278/isms.2017.TA04

Copyright and License Information

Copyright 2017 DeWayne T. Halfen

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