2018ApJ...861...70A


Query : 2018ApJ...861...70A

2018ApJ...861...70A - Astrophys. J., 861, 70-70 (2018/July-1)

Glycinamide, a glycine precursor, caught in the gas phase: a laser-ablation jet-cooled rotational study.

ALONSO E.R., KOLESNIKOVA L., BIALKOWSKA-JAWORSKA E., KISIEL Z., LEON I., GUILLEMIN J.-C. and ALONSO J.L.

Abstract (from CDS):

Glycinamide, a glycine precursor, has been successfully generated in the gas phase by laser ablation of its hydrochloride salt, and its microwave spectrum, recorded from 6 to 16 GHz using a Chirped Pulse Fourier Transform Microwave (LA-CP-FTMW) spectrometer, is reported for the first time. The existence of a single structure stabilized by a Na-H ... NtH2 hydrogen bond has been revealed in the supersonic expansion. The complex nuclear quadrupole coupling hyperfine structure due to the two 14N nuclei has been completely resolved and analyzed using a Molecular Beam Fourier Transform Microwave spectrometer in combination with laser ablation (LA-MB-FTMW spectrometer). The first precise data obtained on this glycine precursor could be of great importance for possible future identifications in the interstellar medium.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): catalogs - ISM: molecules - molecular data - techniques: spectroscopic

Simbad objects: 1

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Number of rows : 1
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 Sgr B2 (North) Rad 17 47 20.2 -28 22 21           ~ 742 1

Query : 2018ApJ...861...70A

Basic data :
NAME Sgr B2 (North) -- Radio Source
Other object types:
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Rad (DGSW,[MD72]), IR ([GBM93])
ICRS coord. (ep=J2000) :
17 47 20.2 -28 22 21 (Radio) [ ] E ~
FK4 coord. (ep=B1950 eq=1950) :
17 44 10.4 -28 21 19 [ ]
Gal coord. (ep=J2000) :
000.6773 -00.0290 [ ]
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Identifiers (7) :
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NAME Sgr B2 (N) NAME Sgr B2 (North) NAME Sgr B2(N) [MD72] 4
DGSW 68 NAME Sgr B2 FIR 1 [GBM93] FIR 1

References (742 between 1850 and 2026) (Total 742)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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