Astrochemistry during the formation of stars
JK Jørgensen, A Belloche… - Annual Review of …, 2020 - annualreviews.org
Star-forming regions show a rich and varied chemistry, including the presence of complex
organic molecules—in both the cold gas distributed on large scales and the hot regions …
organic molecules—in both the cold gas distributed on large scales and the hot regions …
Formation of complex organic molecules in hot molecular cores through nondiffusive grain-surface and ice-mantle chemistry
A new, more comprehensive model of gas–grain chemistry in hot molecular cores is
presented, in which nondiffusive reaction processes on dust-grain surfaces and in ice …
presented, in which nondiffusive reaction processes on dust-grain surfaces and in ice …
Astrochemical evolution along star formation: overview of the IRAM Large Program ASAI
Evidence is mounting that the small bodies of our Solar system, such as comets and
asteroids, have at least partially inherited their chemical composition from the first phases of …
asteroids, have at least partially inherited their chemical composition from the first phases of …
The ALMA-PILS survey: isotopic composition of oxygen-containing complex organic molecules toward IRAS 16293–2422B
Context. One of the important questions of astrochemistry is how complex organic
molecules, including potential prebiotic species, are formed in the envelopes around …
molecules, including potential prebiotic species, are formed in the envelopes around …
The ALMA-PILS survey: inventory of complex organic molecules towards IRAS 16293–2422 A
Context. Complex organic molecules are detected in many sources in the warm inner
regions of envelopes surrounding deeply embedded protostars. Exactly how these species …
regions of envelopes surrounding deeply embedded protostars. Exactly how these species …
Seeds of life in space (SOLIS): the organic composition diversity at 300–1000 au scale in solar-type star-forming regions
C Ceccarelli, P Caselli, F Fontani, R Neri… - The Astrophysical …, 2017 - iopscience.iop.org
Complex organic molecules have been observed for decades in the interstellar medium.
Some of them might be considered as small bricks of the macromolecules at the base of …
Some of them might be considered as small bricks of the macromolecules at the base of …
Ingredients for solar-like systems: protostar IRAS 16293-2422 B versus comet 67P/Churyumov–Gerasimenko
MN Drozdovskaya, EF van Dishoeck… - Monthly Notices of …, 2019 - academic.oup.com
ABSTRACT Our modern day Solar System has 4.6× 109 yr of evolution behind it with just a
few relics of its birth conditions remaining. Comets are thought to be some of the most …
few relics of its birth conditions remaining. Comets are thought to be some of the most …
The ice composition in the disk around V883 Ori revealed by its stellar outburst
Complex organic molecules (COMs), which are the seeds of prebiotic material and
precursors of amino acids and sugars, form in the icy mantles of circumstellar dust grains but …
precursors of amino acids and sugars, form in the icy mantles of circumstellar dust grains but …
A Search for Heterocycles in GOTHAM Observations of TMC-1
We have conducted an extensive search for nitrogen-, oxygen-, and sulfur-bearing
heterocycles toward Taurus Molecular Cloud 1 (TMC-1) using the deep, broadband …
heterocycles toward Taurus Molecular Cloud 1 (TMC-1) using the deep, broadband …
Complex organic molecules in low-mass protostars on Solar System scales-I. Oxygen-bearing species
ML Van Gelder, B Tabone, EF van Dishoeck… - Astronomy & …, 2020 - aanda.org
Context. Complex organic molecules (COMs) are thought to form on icy dust grains in the
earliest phase of star formation. The evolution of these COMs from the youngest Class 0/I …
earliest phase of star formation. The evolution of these COMs from the youngest Class 0/I …