First glycine isomer detected in the interstellar medium: glycolamide (NH2C (O) CH2OH)
We report the first detection in the interstellar medium (ISM) of a C 2 H 5 O 2 N isomer: syn-
glycolamide (NH 2 C (O) CH 2 OH). The exquisite sensitivity at sub-mK levels of an …
glycolamide (NH 2 C (O) CH 2 OH). The exquisite sensitivity at sub-mK levels of an …
Amides inventory towards the G+ 0.693− 0.027 molecular cloud
S Zeng, VM Rivilla, I Jiménez-Serra… - Monthly Notices of …, 2023 - academic.oup.com
Interstellar amides have attracted significant attentions as they are potential precursors for a
wide variety of organics essential to life. However, our current understanding of their …
wide variety of organics essential to life. However, our current understanding of their …
Laboratory spectroscopy of allylimine and tentative detection towards the G+ 0.693-0.027 molecular cloud
Context. Substituted methanimines and ethylenes have been identified in the interstellar
medium. Therefore, allylimine (CH 2= CH–CH= NH) represents a promising candidate for a …
medium. Therefore, allylimine (CH 2= CH–CH= NH) represents a promising candidate for a …
Millimetre and submillimetre spectroscopy of isobutene and its detection in the molecular cloud G+ 0.693
M Fatima, HSP Müller, O Zingsheim, F Lewen… - Astronomy & …, 2023 - aanda.org
Context. Isobutene ((CH 3) 2 C= CH 2) is one of the four isomers of butene (C 4 H 8). Given
the detection of propene (CH 3 CH= CH 2) toward TMC-1, and also in the warmer …
the detection of propene (CH 3 CH= CH 2) toward TMC-1, and also in the warmer …
The first detection of SiC2 in the interstellar medium
S Massalkhi, I Jiménez-Serra, J Martín-Pintado… - Astronomy & …, 2023 - aanda.org
We report the first detection of SiC 2 in the interstellar medium. The molecule was identified
through six rotational transitions toward G+ 0.693-0.027, a molecular cloud located in the …
through six rotational transitions toward G+ 0.693-0.027, a molecular cloud located in the …
On the Formation of Vinylamine (C2H3NH2) in Interstellar Ice Analogs
C Zhang, J Wang, AM Turner, JH Marks… - The Astrophysical …, 2023 - iopscience.iop.org
Amines—organic molecules carrying the–NH 2 moiety—have been recognized as a vital
intermediate in the formation of prebiotic molecules such as amino acids and nucleobases …
intermediate in the formation of prebiotic molecules such as amino acids and nucleobases …
H2CN/H2NC abundance ratio: a new potential temperature tracer for the interstellar medium
The H2NC radical is the high-energy metastable isomer of H2CN radical, which has been
recently detected for the first time in the interstellar medium towards a handful of cold …
recently detected for the first time in the interstellar medium towards a handful of cold …
The complex (organic) puzzle of the formation of hydrogen cyanide and isocyanide on interstellar ice analogues
J Enrique-Romero, T Lamberts - The Journal of Physical …, 2024 - ACS Publications
Aiming to constrain the surface formation of HCN and HNC in the dense interstellar medium
on ice-covered dust grains, we investigate the interaction of CN radicals with H2O and CO …
on ice-covered dust grains, we investigate the interaction of CN radicals with H2O and CO …
Computational Protocol for the Identification of Candidates for Radioastronomical Detection and Its Application to the C3H3NO Family of Isomers
The C3H3NO family of isomers is relevant in astrochemistry, even though its members are
still elusive in the interstellar medium. To identify the best candidate for astronomical …
still elusive in the interstellar medium. To identify the best candidate for astronomical …
Discovery of Thionylimide, HNSO, in Space: The first N-, S-, and O-bearing Interstellar Molecule
M Sanz-Novo, VM Rivilla, HSP Müller… - The Astrophysical …, 2024 - iopscience.iop.org
We present the first detection in space of thionylimide (HNSO) toward the Galactic center
molecular cloud G+ 0.693-0.027, thanks to the superb sensitivity of an ultradeep molecular …
molecular cloud G+ 0.693-0.027, thanks to the superb sensitivity of an ultradeep molecular …