Search Results - "Wakelam, V."
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FROM PRESTELLAR TO PROTOSTELLAR CORES. II. TIME DEPENDENCE AND DEUTERIUM FRACTIONATION
Published in The Astrophysical journal (20-11-2012)“…We investigate the molecular evolution and D/H abundance ratios that develop as star formation proceeds from a dense molecular cloud core to a protostellar…”
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Modelling complex organic molecules in dense regions: Eley–Rideal and complex induced reaction
Published in Monthly notices of the Royal Astronomical Society (11-03-2015)“…Recent observations have revealed the existence of complex organic molecules (COMs) in cold dense cores and pre-stellar cores. The presence of these molecules…”
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Predictions of gas-phase methanimine (CH2NH) abundance in cold cores
Published in Monthly notices of the Royal Astronomical Society (01-05-2023)“…ABSTRACT Since the 1930s, more than 250 molecules have been discovered in the interstellar medium. With the development of more sensitive telescopes, we keep…”
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CHEMICAL AND PHYSICAL CHARACTERIZATION OF COLLAPSING LOW-MASS PRESTELLAR DENSE CORES
Published in The Astrophysical journal (01-05-2016)“…ABSTRACT The first hydrostatic core, also called the first Larson core, is one of the first steps in low-mass star formation as predicted by theory. With…”
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Grain-surface reactions in molecular clouds: the effect of cosmic rays and quantum tunnelling
Published in Monthly notices of the Royal Astronomical Society (01-06-2014)“…Grain-surface reactions play an essential role in interstellar chemistry, since dust grain catalyzes reactions at its surface allowing for the formation of…”
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Polysulphanes on interstellar grains as a possible reservoir of interstellar sulphur
Published in Monthly notices of the Royal Astronomical Society (11-10-2012)“…Abstract The form of depleted sulphur in dense clouds is still unknown. Until now, only two molecules, OCS and SO2, have been detected in interstellar ices but…”
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Sulphur chemistry in the L1544 pre-stellar core
Published in Monthly notices of the Royal Astronomical Society (21-08-2018)“…ABSTRACT The L1544 pre-stellar core has been observed as part of the ASAI IRAM 30 m Large Program as well as follow-up programs. These observations have…”
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SURVIVAL OF INTERSTELLAR MOLECULES TO PRESTELLAR DENSE CORE COLLAPSE AND EARLY PHASES OF DISK FORMATION
Published in The Astrophysical journal (20-09-2013)“…An outstanding question of astrobiology is the link between the chemical composition of planets, comets, and other solar system bodies and the molecules formed…”
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LEGO – II. A 3 mm molecular line study covering 100 pc of one of the most actively star-forming portions within the Milky Way disc
Published in Monthly notices of the Royal Astronomical Society (11-09-2020)“…ABSTRACT The current generation of (sub)mm-telescopes has allowed molecular line emission to become a major tool for studying the physical, kinematic, and…”
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A fast neural emulator for interstellar chemistry
Published in Monthly notices of the Royal Astronomical Society (14-07-2024)“…ABSTRACT Astrochemical models are important tools to interpret observations of molecular and atomic species in different environments. However, these models…”
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3D modelling of HCO+ and its isotopologues in the low-mass proto-star IRAS16293−2422
Published in Monthly notices of the Royal Astronomical Society (01-07-2018)“…Abstract Ions and electrons play an important role in various stages of the star formation process. By following the magnetic field of their environment and…”
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A study of singly deuterated cyclopropenylidene c-C3HD in the protostar IRAS 16293–2422
Published in Monthly notices of the Royal Astronomical Society (01-06-2017)“…Abstract Cyclic-C3HD (c-C3HD) is a singly deuterated isotopologue of c-C3H2, which is one of the most abundant and widespread molecules in our Galaxy. We…”
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Influence of galactic arm scale dynamics on the molecular composition of the cold and dense ISM – II. Molecular oxygen abundance
Published in Monthly notices of the Royal Astronomical Society (01-07-2019)“…ABSTRACT Molecular oxygen has been the subject of many observational searches as chemical models predicted it to be a reservoir of oxygen. Although it has been…”
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Detection of CH3SH in protostar IRAS 16293-2422
Published in Monthly notices of the Royal Astronomical Society (11-05-2016)“…The nature of the main sulphur reservoir in star forming regions is a long standing mystery. The observed abundance of sulphur-bearing species in dense clouds…”
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Protoplanetary discs: sensitivity of the chemical composition to various model parameters
Published in Monthly notices of the Royal Astronomical Society (01-04-2019)“…Protoplanetary disks are challenging objects for astrochemical models due to strong density and temperature gradients and due to the UV photons 2D propagation…”
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Detection of HOCO+ in the protostar IRAS 16293−2422
Published in Monthly notices of the Royal Astronomical Society (11-06-2018)“…Abstract The protonated form of CO2, HOCO+, is assumed to be an indirect tracer of CO2 in the millimeter/submillimeter regime since CO2 lacks a permanent…”
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Chemical modelling of water deuteration in IRAS16293-2422
Published in Monthly notices of the Royal Astronomical Society (11-12-2014)“…IRAS 16293-2422 is a well-studied low-mass protostar characterized by a strong level of deuterium fractionation. In the line of sight of the protostellar…”
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Methyl isocyanate (CH3NCO): an important missing organic in current astrochemical networks
Published in Monthly notices of the Royal Astronomical Society. Letters (01-01-2018)“…Abstract Methyl isocyanate (CH3NCO) is one of the important complex organic molecules detected on the comet 67P/Churyumov–Gerasimenko by Rosetta’s Philae…”
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SiS Formation in the Interstellar Medium through Si+SH Gas-phase Reactions
Published in The Astrophysical journal (11-10-2021)“…Abstract Silicon monosulfide is an important silicon-bearing molecule detected in circumstellar envelopes and star-forming regions. Its formation and…”
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The Hot Core around the Low-Mass Protostar IRAS 16293–2422: Scoundrels Rule
Published in The Astrophysical journal (10-08-2003)Get full text
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