activity
20222026
most citedTracing the contraction of the pre-stellar core L1544 with HCO = 1-0 emission

7 citations · 13 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Inventories of Rich Carbon-Chain Chemistry in Prestellar and Starless Cores in the Perseus Molecular Cloud

Anissa Pokorny-Yadav, Samantha Scibelli, Judit Ferrer Asensio +3

Carbon-chain molecules serve as an important reservoir of reactive organic matter that will eventually be incorporated into protoplanetary disks, planets, and cometary material. Pr…

astro-ph.GA2026

c-C3H2 deuteration towards prestellar and starless cores in the Perseus Molecular Cloud

J. Ferrer Asensio, S. Scibelli, L. Steffes +6

Deuterium fractionation becomes highly efficient in cold, dense cores where CO is frozen out. Cyclopropenylidene (c-C3H2), an early-formed carbon ring, and its deuterated isotopolo…

astro-ph.GA20256 cited

Nascent chemical complexity in prestellar core IRAS 16293E: complex organics and deuterated methanol

Samantha Scibelli, Maria N. Drozdovskaya, Paola Caselli +5

Prestellar cores represent early sites of low-mass ( few M) star and planet formation and provide insight into initial chemical conditions of complex organic mole…

astro-ph.GA2024

Fractionation in young cores: Direct determinations of nitrogen and carbon fractionation in HCN

S. S. Jensen, S. Spezzano, P. Caselli +4

We aim to determine the N/N and C/C ratios for HCN in six starless and prestellar cores and compare the results between the direct method using radiativ…

astro-ph.GA2024

A deep search for large complex organic species toward IRAS16293-2422 B at 3 mm with ALMA

P. Nazari, J. S. Y. Cheung, J. Ferrer Asensio +14

Complex organic molecules (COMs) have been detected ubiquitously in protostellar systems. However, at shorter wavelengths (~0.8mm) it is more difficult to detect larger molecules t…

astro-ph.GA20227 cited

Tracing the contraction of the pre-stellar core L1544 with HCO = 1-0 emission

J. Ferrer Asensio, S. Spezzano, P. Caselli +6

Spectral line profiles of several molecules observed towards the pre-stellar core L1544 appear double-peaked. For abundant molecular species this line morphology has been linked to…