[HTML][HTML] CoCCoA: Complex Chemistry in hot Cores with ALMA-Selected oxygen-bearing species

Y Chen, ML Van Gelder, P Nazari, CL Brogan… - Astronomy & …, 2023 - aanda.org
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 …

Photodissociation and photoionization of molecules of astronomical interest-Updates to the Leiden photodissociation and photoionization cross section database

HR Hrodmarsson, EF Van Dishoeck - Astronomy & Astrophysics, 2023 - aanda.org
Context. Vacuum-ultraviolet (VUV) photons are important drivers of chemical processes in
space. Thus, it is important to accurately characterize and constrain photorates in different …

FAUST–VIII. The protostellar disc of VLA 1623–2417W and its streamers imaged by ALMA

S Mercimek, L Podio, C Codella… - Monthly Notices of …, 2023 - academic.oup.com
More than 50 per cent of solar-mass stars form in multiple systems. It is therefore crucial to
investigate how multiplicity affects the star and planet formation processes at the protostellar …

FAUST XII. Accretion streamers and jets in the VLA 1623–2417 protocluster

C Codella, L Podio, M De Simone… - Monthly Notices of …, 2024 - academic.oup.com
The ALMA interferometer has played a key role in revealing a new component of the Sun-
like star forming process: the molecular streamers, ie structures up to thousands of au long …

FAUST. VII. Detection of a Hot Corino in the Prototypical Warm Carbon-chain Chemistry Source IRAS 15398–3359

Y Okoda, Y Oya, L Francis, D Johnstone… - The Astrophysical …, 2023 - iopscience.iop.org
We have observed the low-mass protostellar source IRAS 15398− 3359 at a resolution of 0
farcs 2–0 farcs 3, as part of the Atacama Large Millimeter/Submillimeter Array Large …

FAUST. XIV. Probing the Flared Disk in L1527 with Sulfur-bearing Molecules

ZE Zhang, N Sakai, S Ohashi, NM Murillo… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract IRAS04368+ 2557 in L1527 is a Class 0/I protostar with a clear disk-envelope
system revealed by previous Atacama Large Millimeter/submillimeter Array (ALMA) …

Correlations among complex organic molecules around protostars: Effects of physical structure

P Nazari, B Tabone, GP Rosotti… - arXiv preprint arXiv …, 2024 - aanda.org
Context. Complex organic molecules have been observed toward many protostars. Their
column density ratios are generally constant across protostellar systems, with some low …

Molecular complexity of young solar analogues

E Bianchi, M De Simone, G Sabatini, J Frediani… - arXiv preprint arXiv …, 2024 - arxiv.org
How does molecular complexity emerge and evolve during the process leading to the
formation of a planetary system? Astrochemistry is experiencing a golden age, marked by …

The ALMA Legacy survey of Class 0/I disks in Corona australis, Aquila, chaMaeleon, oPhiuchus north, Ophiuchus, Serpens (CAMPOS). I. Evolution of Protostellar disk …

CH Hsieh, HG Arce, MJ Maureira, JE Pineda… - arXiv preprint arXiv …, 2024 - arxiv.org
We surveyed nearly all the embedded protostars in seven nearby clouds (Corona Australis,
Aquila, Chamaeleon I & II, Ophiuchus North, Ophiuchus, Serpens) with the Atacama Large …

[PDF][PDF] Bridging the gap bet een ph sics and chemistr in earl stages of star formation

P Nazari - A&A, 2022 - scholarlypublications …
Context. Complex organic species are known to be abundant toward low-and high-mass
protostars. No statistical study of these species toward a large sample of high-mass …