activity
20172022
most citedHot Corinos Chemical Diversity: Myth or Reality?

77 citations · 253 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.GA202232 cited

FAUST III. Misaligned rotations of the envelope, outflow, and disks in the multiple protostellar system of VLA 16232417

Satoshi Ohashi, Claudio Codella, Nami Sakai +69

We report a study of the low-mass Class-0 multiple system VLA 1623AB in the Ophiuchus star-forming region, using HCO (), CS (), and CCH () lines as…

astro-ph.SR202139 cited

FAUST II. Discovery of a Secondary Outflow in IRAS 15398-3359: Variability in Outflow Direction during the Earliest Stage of Star Formation?

Yuki Okoda, Yoko Oya, Logan Francis +66

We have observed the very low-mass Class 0 protostar IRAS 15398-3359 at scales ranging from 50 au to 1800 au, as part of the ALMA Large Program FAUST. We uncover a linear feature,…

astro-ph.SR202051 cited

FAUST I. The hot corino at the heart of the prototypical Class I protostar L1551 IRS5

E. Bianchi, C. J. Chandler, C. Ceccarelli +63

The study of hot corinos in Solar-like protostars has been so far mostly limited to the Class 0 phase, hampering our understanding of their origin and evolution. In addition, recen…

astro-ph.SR202077 cited

Hot Corinos Chemical Diversity: Myth or Reality?

Marta De Simone, Cecilia Ceccarelli, Claudio Codella +14

After almost 20 years of hunting, only about a dozen hot corinos, hot regions enriched in interstellar complex organic molecules (iCOMs), are known. Of them, many are binary system…

astro-ph.GA202023 cited

The MUSTANG-2 Galactic Plane Survey (MGPS90) pilot

Adam Ginsburg, L. D. Anderson, Simon Dicker +19

We report the results of a pilot program for a Green Bank Telescope (GBT) MUSTANG Galactic Plane survey at 3 mm (90 GHz), MGPS90. The survey achieves a typical depth of

astro-ph.GA2019

ALMA observations of fragmentation, sub-structure, and protostars in high-mass starless clump candidates

Brian E. Svoboda, Yancy L. Shirley, Alessio Traficante +7

(Abridged) The initial physical conditions of high-mass stars and protoclusters remain poorly characterized. To this end we present the first targeted ALMA 1.3mm continuum and spec…