most citedModest dust settling in the IRAS04302+2247 Class I protoplanetary disk

36 citations · 101 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2023

Protostellar chimney flues: are jets and outflows lifting submillimetre dust grains from discs into envelopes?

L. Cacciapuoti, L. Testi, L. Podio +7

Low dust opacity spectral indices () measured in the inner envelopes of class 0/I young stellar objects (age yr) have been interpreted as the presence of (sub…

astro-ph.SR202325 cited

FAUST VIII. The protostellar disk of VLA 1623-2417 W and its streamers imaged by ALMA

S. Mercimek, L. Podio, C. Codella +25

More than 50% of solar-mass stars form in multiple systems. It is therefore crucial to investigate how multiplicity affects the star and planet formation processes at the protostel…

astro-ph.SR202314 cited

FAUST VII. Detection of A Hot Corino in the Prototypical Warm Carbon-Chain Chemistry Source IRAS 15398-3359

Yuki Okoda, Yoko Oya, Logan Francis +16

We have observed the low-mass protostellar source, IRAS 153983359, at a resolution of 0.2-0.3, as part of the Atacama Large Millimeter/Submillimeter Array Large Program…

astro-ph.SR202336 cited

Modest dust settling in the IRAS04302+2247 Class I protoplanetary disk

M. Villenave, L. Podio, G. Duchene +11

We present new VLA observations, between 6.8mm and 66mm, of the edge-on Class~I disk IRAS04302+2247. Observations at 6.8mm and 9.2mm lead to the detection of thermal emission from…

astro-ph.SR202212 cited

Tracking the ice mantle history in the Solar-type Protostars of NGC 1333 IRAS 4

Marta De Simone, Cecilia Ceccarelli, Claudio Codella +13

To understand the origin of the diversity observed in exoplanetary systems, it is crucial to characterize the early stages of their formation, represented by Solar-type protostars.…

astro-ph.GA202214 cited

FAUST VI. VLA 1623--2417 B: a new laboratory for astrochemistry around protostars on 50 au scale

C. Codella, A. López-Sepulcre, S. Ohashi +25

The ALMA interferometer, with its unprecedented combination of high-sensitivity and high-angular resolution, allows for (sub-)mm wavelength mapping of protostellar systems at Solar…