Cometary Chemistry and the Origin of Icy Solar System Bodies: The View After Rosetta

K Altwegg, H Balsiger, SA Fuselier - Annual Review of …, 2019 - annualreviews.org
In situ research of cometary chemistry began when measurements from the Giotto mission at
Comet 1P/Halley revealed the presence of complex organics in the coma. New telescopes …

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 …

Prebiotic chemicals—amino acid and phosphorus—in the coma of comet 67P/Churyumov-Gerasimenko

K Altwegg, H Balsiger, A Bar-Nun, JJ Berthelier… - Science …, 2016 - science.org
The importance of comets for the origin of life on Earth has been advocated for many
decades. Amino acids are key ingredients in chemistry, leading to life as we know it. Many …

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 …

Sources of Nitrogen-, Sulfur-, and Phosphorus-containing feedstocks for prebiotic chemistry in the planetary environment

ZR Todd - Life, 2022 - mdpi.com
Biochemistry on Earth makes use of the key elements carbon, hydrogen, oxygen, nitrogen,
phosphorus, and sulfur (or CHONPS). Chemically accessible molecules containing these …

Ionize Hard: Interstellar PO+ Detection

VM Rivilla, J García De La Concepción… - Frontiers in Astronomy …, 2022 - frontiersin.org
We report the first detection of the phosphorus monoxide ion (PO+) in the interstellar
medium. Our unbiased and very sensitive spectral survey toward the G+ 0.693–0.027 …

Chemical equilibrium in AGB atmospheres: successes, failures, and prospects for small molecules, clusters, and condensates

M Agúndez, JI Martínez, PL de Andres… - Astronomy & …, 2020 - aanda.org
Chemical equilibrium has proven extremely useful for predicting the chemical composition of
AGB atmospheres. Here we use a recently developed code and an updated thermochemical …

ALMA and ROSINA detections of phosphorus-bearing molecules: the interstellar thread between star-forming regions and comets

VM Rivilla, MN Drozdovskaya, K Altwegg… - Monthly Notices of …, 2020 - academic.oup.com
To understand how phosphorus (P)-bearing molecules are formed in star-forming regions,
we have analysed the Atacama Large Millimeter/Submillimeter Array (ALMA) observations …

New molecules in IRC+ 10216: confirmation of C5S and tentative identification of MgCCH, NCCP, and SiH3CN

M Agúndez, J Cernicharo, M Guélin - Astronomy & Astrophysics, 2014 - aanda.org
The carbon-star envelope IRC+ 10216 harbors a rich variety of molecules, with more than
80 detected to date. During the course of a λ 3 mm survey of IRC+ 10216 carried out with the …

Confirmation of circumstellar phosphine

M Agúndez, J Cernicharo, L Decin… - The Astrophysical …, 2014 - iopscience.iop.org
Phosphine (PH 3) was tentatively identified a few years ago in the carbon star envelopes
IRC+ 10216 and CRL 2688 from observations of an emission line at 266.9 GHz attributable …