2021ApJ...914..136C


Query : 2021ApJ...914..136C

2021ApJ...914..136C - Astrophys. J., 914, 136-136 (2021/June-3)

Can cytosine, uracil, and thymine be formed from HC3N and H2NCO+ in interstellar space?

CHOE J.C.

Abstract (from CDS):

Syntheses of cytosine, uracil, and thymine starting from interstellar molecules were examined theoretically. Potential energy surfaces for the formation of protonated cytosine (CyH+), uracil (UrH+), and thymine (ThH+) from cyanoacetylene (HC3N), protonated isocyanic acid (H2NCO+), and one of NH3, H2O, and CH3OH, respectively, were determined by quantum chemical calculation using the CBS-QB3 method. Barrierless pathways were found for all the three reactions. Investigation of the energetics and kinetics of further possible reactions of CyH+, UrH+, and ThH+ led to the conclusion that cytosine, uracil, and thymine could not be formed along the proposed pathways in the interstellar gas phase, whereas their formation might be possible on interstellar icy grain mantles.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Interstellar medium - Interstellar molecules - Astrobiology - Astrochemistry

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0
2 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 2443 1
3 LDN 483 DNe 18 17 35 -04 39.8           ~ 359 0

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