activity
20202026
most citedALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT) VI: Accretion shocks in the disk of DG Tau and HL Tau

106 citations · 541 across the 19 of their papers we have counts for

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astro-ph.GA2020★ 45 cited

ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT) V: Sample, overview, and demography of disk molecular emission

Antonio Garufi, Linda Podio, Claudio Codella +9

We present an overview of the ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT), a campaign devoted to the characterization of the molecular emission from partly em…

astro-ph.GA2020★ 16 cited

ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT) III: The interplay between gas and dust in the protoplanetary disk of DG Tau

L. Podio, A. Garufi, C. Codella +9

Planets form in protoplanetary disks and inherit their chemical composition. It is therefore crucial to understand the disks molecular content. We aim to characterize the distribut…

astro-ph.EP2020★ 9 cited

ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT). IV. Thioformaldehyde (HCS) in protoplanetary disks: spatial distributions and binding energies

C. Codella, L. Podio, A. Garufi +10

Aims: To trace the radial and vertical spatial distribution of H2CS, a key species of the S-bearing chemistry, in protoplanetary disks. To analyse the observed distributions in lig…

astro-ph.SR2020★ 66 cited

ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT) II: Vertical stratification of CO, CS, CN, HCO, and CHOH in a Class I disk

L. Podio, A. Garufi, C. Codella +8

The chemical composition of planets is inherited from that of the protoplanetary disk at the time of planet formation. Increasing observational evidence suggests that planet format…

astro-ph.SR2020★ 51 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…