activity
20062022
most citedCO Isotopologues in the Perseus Molecular Cloud Complex: the X-Factor and Regional Variations

303 citations · 6.1k across the 101 of their papers we have counts for

collaborators

102 papers

astro-ph.GA2022★ 22 cited

Hot methanol in the [BHB2007] 11 protobinary system: hot corino versus shock origin? : FAUST V

C. Vastel, F. Alves, C. Ceccarelli +63

Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the building-up of the chemical complexity in star formi…

astro-ph.IM2022★ 97 cited

pyspeckit: A spectroscopic analysis and plotting package

Adam Ginsburg, Vlas Sokolov, Miguel de Val-Borro +4

pyspeckit is a toolkit and library for spectroscopic analysis in Python. We describe the pyspeckit package and highlight some of its capabilities, such as interactively fitting a m…

astro-ph.GA2022★ 35 cited

An Interferometric View of H-MM1. I. Direct Observation of NH3 Depletion

Jaime E. Pineda, Jorma Harju, Paola Caselli +14

Spectral lines of ammonia, NH, are useful probes of the physical conditions in dense molecular cloud cores. In addition to advantages in spectroscopy, ammonia has also been sug…

astro-ph.GA2022

From Bubbles and Filaments to Cores and Disks: Gas Gathering and Growth of Structure Leading to the Formation of Stellar Systems

Jaime E. Pineda, Doris Arzoumanian, Philippe André +8

The study of the development of structures on multiple scales in the cold interstellar medium has experienced rapid expansion in the past decade, on both the observational and the…

astro-ph.SR2022★ 14 cited

Mass ejection and time variability in protostellar outflows: Cep E. SOLIS XVI

A. de A. Schutzer, P. R. Rivera-Ortiz, B. Lefloch +46

Protostellar jets are an important agent of star formation feedback, tightly connected with the mass-accretion process. The history of jet formation and mass-ejection provides cons…

astro-ph.SR2022★ 80 cited

The Central 1000 au of a Pre-stellar Core Revealed with ALMA. II. Almost Complete Freeze-out

Paola Caselli, Jaime E. Pineda, Olli Sipilä +18

Pre-stellar cores represent the initial conditions in the process of star and planet formation. Their low temperatures (10 K) allow the formation of thick icy dust mantles, whic…