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20242026
most citedChemical complexity in star formation induced by stellar feedback: cores shock-formed by the supernova remnant W44

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astro-ph.GA2024

Interaction between the Supernova Remnant W44 and the Infrared Dark Cloud G034.77-00.55: shock induced star formation?

G. Cosentino, I. Jiménez-Serra, A. T. Barnes +11

How Supernova Remnant (SNR) shocks impact nearby molecular clouds is still poorly observationally constrained. It is unclear if SNRs can positively or negatively affect clouds star…

astro-ph.GA2024

The SOFIA Massive (SOMA) Star Formation Q-band follow-up I. Carbon-chain chemistry of intermediate-mass protostars

Kotomi Taniguchi, Prasanta Gorai, Jonathan C. Tan +10

Evidence for similar chemical characteristics around low- and high-mass protostars has been found: in particular, a variety of carbon-chain species and complex organic molecules (C…

astro-ph.GA2024

The ALMA-QUARKS Survey: Fibers' role in star formation unveiled in an intermediate-mass protocluster region of the Vela D cloud

Dongting Yang, HongLi Liu, Tie Liu +32

In this paper, we present a detailed analysis of the IRS 17 filament within the intermediate-mass protocluster IRAS 08448-4343 (of ), using ALMA data fro…

astro-ph.GA2024

Assessing realistic binding energies of some essential interstellar radicals with amorphous solid water. A fully quantum chemical approach

Milan Sil, Arghyadeb Roy, Prasanta Gorai +6

In the absence of laboratory data, state-of-the-art quantum chemical approaches can provide estimates of the binding energy (BE) of interstellar species with grains. Without BE val…

astro-ph.GA2024

Carbon-Chain Chemistry in the Interstellar Medium

Kotomi Taniguchi, Prasanta Gorai, Jonathan C. Tan

The presence of carbon-chain molecules in the interstellar medium (ISM) has been known since the early 1970s and such species have been identified to date, making up $\sim 4…