activity
20222026
most citedHunt for complex cyanides in protostellar ices with JWST: Tentative detection of CHCN and CHCN

43 citations · 107 across the 5 of their papers we have counts for

collaborators

6 papers

physics.ed-ph2026

Using Learning Analytics to Study Novice Learners' Work on Quantum Circuit Simulator Tasks

Juuso Jaakola, Vlad Stirbu, Teiko Heinosaari

Interactive quantum circuit simulators are increasingly used to support introductory quantum computing education for learners from varied disciplinary backgrounds. These environmen…

astro-ph.GA2025★ 3 cited

SOFIA FIFI-LS spectroscopy of DR21 Main: energetics of the spatially-resolved outflow from a high-mass protostar

A. Karska, M. Figueira, A. Mirocha +12

Massive star formation is associated with energetic processes that may influence the physics and chemistry of parental molecular clouds and impact galaxy evolution. The high-mass p…

astro-ph.GA2024★ 3 cited

The factors that influence protostellar multiplicity I: Gas temperature, density, and mass in Perseus with Nobeyama

N. M. Murillo, C. M. Fuchs, D. Harsono +9

Protostellar multiplicity is common at all stages and mass ranges. However, the factors that determine the multiplicity of protostellar systems have not been systematically charact…

astro-ph.GA2024★ 43 cited

Hunt for complex cyanides in protostellar ices with JWST: Tentative detection of CHCN and CHCN

P. Nazari, W. R. M. Rocha, A. E. Rubinstein +20

Nitrogen-bearing complex organic molecules have been commonly detected in the gas phase but not yet in interstellar ices. This has led to the long-standing question of whether thes…

astro-ph.SR2023★ 30 cited

The Perseus ALMA Chemical Survey (PEACHES). III. Sulfur-bearing species tracing accretion and ejection processes in young protostars

E. Artur de la Villarmois, V. V. Guzman, Y. -L. Yang +2

(Abridged) Sulfur chemistry is poorly understood in the process of low-mass star and planet formation, where the main carriers of sulfur are still unknown. Despite the fact that si…

astro-ph.SR2022★ 28 cited

Importance of source structure on complex organics emission. I. Observations of CHOH from low-mass to high-mass protostars

M. L. van Gelder, P. Nazari, B. Tabone +9

Complex organic molecules (COMs) are often observed toward embedded Class 0 and I protostars. However, not all Class 0 and I protostars exhibit COMs emission. In this work, variati…