activity
20152023
most citedThe ALMA Protostellar Interferometric Line Survey (PILS): First results from an unbiased submillimeter wavelength line survey of the Class 0 protostellar binary IRAS 16293-2422 with ALMA

402 citations · 1.7k across the 37 of their papers we have counts for

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Showing 2021Show all

5 papers · 1 filter

astro-ph.GA2021★ 31 cited

Organic chemistry in the protosolar analogue HOPS-108: Environment matters

L. Chahine, A. López-Sepulcre, R. Neri +10

Hot corinos are compact regions around solar-mass protostellar objects that are very rich in interstellar complex organic molecules (iCOMs). They are believed to represent the very…

astro-ph.GA2021★ 5 cited

Seeds of Life in Space (SOLIS). XIII. Nitrogen fractionation towards the protocluster OMC-2 FIR4

Lucy Evans, Francesco Fontani, Charlotte Vastel +8

Isotopic fractionation is an important tool to investigate the chemical history of our Solar System (SS). In particular, the isotopic fraction of nitrogen (14N/15N) is lower in com…

astro-ph.GA2021★ 22 cited

The SVS13-A Class I chemical complexity as revealed by S-bearing species. SOLIS XIII

C. Codella, E. Bianchi, L. Podio +13

Aims: The goal is to obtain a census of S-bearing species using interferometric images, towards SVS13-A, a Class I object associated with a hot corino rich in interstellar complex…

astro-ph.GA2021

Rotating Motion of the Outflow of IRAS 16293-2422 A1 at its Origin Point near the Protostar

Yoko Oya, Yoshimasa Watanabe, Ana López-Sepulcre +4

The Class 0 protostar IRAS 162932422 Source A is known to be a binary system (A1 and A2) or even a multiple system, which processes a complex outflow structure. We have observed…

astro-ph.SR2021★ 39 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,…