2018 census of interstellar, circumstellar, extragalactic, protoplanetary disk, and exoplanetary molecules
BA McGuire - The Astrophysical Journal Supplement Series, 2018 - iopscience.iop.org
To date, 204 individual molecular species, comprised of 16 different elements, have been
detected in the interstellar and circumstellar medium by astronomical observations. These …
detected in the interstellar and circumstellar medium by astronomical observations. These …
2021 census of interstellar, circumstellar, extragalactic, protoplanetary disk, and exoplanetary molecules
BA McGuire - The Astrophysical Journal Supplement Series, 2022 - iopscience.iop.org
To date, 241 individual molecular species, composed of 19 different elements, have been
detected in the interstellar and circumstellar medium by astronomical observations. These …
detected in the interstellar and circumstellar medium by astronomical observations. These …
A sensitive λ 3 mm line survey of L483-A broad view of the chemical composition of a core around a Class 0 object
M Agúndez, N Marcelino, J Cernicharo… - Astronomy & …, 2019 - aanda.org
An exhaustive chemical characterization of dense cores is mandatory to our understanding
of chemical composition changes from a starless to a protostellar stage. However, only a few …
of chemical composition changes from a starless to a protostellar stage. However, only a few …
[HTML][HTML] CoCCoA: Complex Chemistry in hot Cores with ALMA-Selected oxygen-bearing species
Context. Complex organic molecules (COMs), especially the oxygen-bearing species, have
been observed to be abundant in the gas phase toward low-mass and high-mass protostars …
been observed to be abundant in the gas phase toward low-mass and high-mass protostars …
Search for high-mass protostars with alma revealed up to kilo-parsec scales (sparks)-II. Complex organic molecules and heavy water in shocks around a young high …
T Csengeri, A Belloche, S Bontemps… - Astronomy & …, 2019 - aanda.org
Context. Classical hot cores are rich in molecular emission, and they show a high
abundance of complex organic molecules (COMs). The emergence of molecular complexity …
abundance of complex organic molecules (COMs). The emergence of molecular complexity …
Millimeterwave and submillimeterwave laboratory spectroscopy in support of observational astronomy
SL Widicus Weaver - Annual Review of Astronomy and …, 2019 - annualreviews.org
The recent advancements in far-infrared (far-IR) astronomy brought about by the Herschel,
SOFIA, and ALMA observatories have led to technological advancements in millimeterwave …
SOFIA, and ALMA observatories have led to technological advancements in millimeterwave …
The GUAPOS project-III. Characterization of the O-and N-bearing complex organic molecules content and search for chemical differentiation
C Mininni, MT Beltrán, L Colzi, VM Rivilla… - Astronomy & …, 2023 - aanda.org
Context. The G31. 41+ 0.31 Unbiased ALMA sPectral Observational Survey (GUAPOS)
project targets the hot molecular core (HMC) G31. 41+ 0.31 (G31) to reveal the complex …
project targets the hot molecular core (HMC) G31. 41+ 0.31 (G31) to reveal the complex …
An ALCHEMI inspection of sulphur-bearing species towards the central molecular zone of NGC 253
M Bouvier, S Viti, E Behrens, J Butterworth… - Astronomy & …, 2024 - aanda.org
Context. Sulphur-bearing species are detected in various environments within Galactic star-
forming regions and are particularly abundant in the gas phase of outflow and shocked …
forming regions and are particularly abundant in the gas phase of outflow and shocked …
The prebiotic molecular inventory of Serpens SMM1: II. The building blocks of peptide chains
NFW Ligterink, A Ahmadi, B Luitel… - ACS Earth and Space …, 2022 - ACS Publications
This work aims to constrain the abundances of interstellar amides, by searching for this
group of prebiotic molecules in the intermediate-mass protostar Serpens SMM1-a. ALMA …
group of prebiotic molecules in the intermediate-mass protostar Serpens SMM1-a. ALMA …
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions – VIII. A search for hot cores by using C2H5CN, CH3OCHO, and CH3OH lines
Hot cores characterized by rich lines of complex organic molecules are considered as ideal
sites for investigating the physical and chemical environments of massive star formation. We …
sites for investigating the physical and chemical environments of massive star formation. We …