2025ApJS..277...14Z


Query : 2025ApJS..277...14Z

2025ApJS..277...14Z - Astrophys. J., Suppl. Ser., 277, 14 (2025/March-0)

Chemistry of NH2CH2CH2OH and Its Related Species in the Interstellar Medium.

ZHAO G., HE M., QUAN D., YANG X., CHEN L.-F., LI D., CHANG Q., WU Y., TENG Y., QIU Y., HE X., MA M.-S. and QU M.

Abstract (from CDS):

Ethanolamine (NH2CH2CH2OH) can form not only glycine directly under the conditions of proposed Archean alkaline hydrothermal vents, a possible environment for the origin of life, but also the polar hydrophilic head of phosphatidylethanolamine, the second most abundant phospholipid in cell membranes, under possible conditions of the primitive Earth. Recently, NH2CH2CH2OH was detected toward the G+0.693-0.027 molecular cloud. We construct the chemical network for NH2CH2CH2OH and its related species (HOCH2CN, CH3NH2, NH2OH, CH3OH, C2H5OH, and C2H3OH) via quantum chemical calculations, simulate their abundance evolutions with the pnautilus code, and then acquire the best-fitting shock-wave model for G+0.693: the combination of isothermal model I5 (Tg = Td = 16 K, nH = 4 × 103 cm–3, AV = 6 mag, and ζ = 1.3 × 10–15 s–1) and continuous shock model S5 (Vs = 20 km s–1). We find NH2CH2CH2OH mainly comes from the thermal desorption produced by shock-induced heating and the photodesorption generated by cosmic-ray-induced UV photons; overall, its ice-phase species is mostly produced by four sequential ice-phase addition pathways, in which the final reactions are J-H + J-NH2CH2CHOH → J-NH2CH2CH2OH, J-H + J-NHCH2CH2OH → J-NH2CH2CH2OH, J-H + J-NH2CH2CH2O → J-NH2CH2CH2OH, and J-CH2OH + J-CH2NH2 → J-NH2CH2CH2OH. We also discuss the formation of HOCH2CN, CH3OH, C2H5OH, and C2H3OH in the best-fitting shock-wave model, as well as the formation of NH2CH2CH2OH in a typical hot-core model. Moreover, we predict NH2CH2CH2OH may be detected toward the newly formed hot core; the undiscovered species CH2CH2OH and HOCCNH are potentially detectable toward G+0.693.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Pre-biotic astrochemistry - Interstellar medium - Interstellar molecules - Theoretical models - Interstellar abundances

Simbad objects: 7

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Number of rows : 7
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 NAME Orion-KL SFR 05 35 14.16 -05 22 21.5           ~ 2421 1
2 NAME IRAS 16293-2422B Y*O 16 32 22.63 -24 28 31.8           ~ 352 0
3 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
4 NAME Sgr B2 (North) Rad 17 47 20.2 -28 22 21           ~ 742 1
5 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 2443 1
6 GCM +0.693 -0.027 MoC 17 47 21.9 -28 21 27           ~ 128 0
7 W 51e2 Ma* 19 23 43.906 +14 30 34.48           ~ 222 0

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