activity
20162026
most citedCharacterizing young protostellar disks with the CALYPSO IRAM-PdBI survey: large Class 0 disks are rare

167 citations · 1.3k across the 31 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

astro-ph.GA2022★ 16 cited

Importance of source structure on complex organics emission III. Effect of disks around massive protostars

P. Nazari, B. Tabone, G. P. Rosotti

Complex organic molecules are only detected toward a fraction of high-mass protostars. The goal of this work is to investigate whether high-mass disks can explain the lack of metha…

astro-ph.EP2022★ 58 cited

Directly tracing the vertical stratification of molecules in protoplanetary disks

T. Paneque-Carreño, A. Miotello, E. F. van Dishoeck +3

We aim to directly trace the vertical location of the emitting surface of multiple molecular tracers in protoplanetary disks. Our sample of disks includes Elias 2-27, WaOph 6 and t…

astro-ph.GA2022★ 48 cited

N-bearing complex organics toward high-mass protostars: Constant ratios pointing to formation in similar pre-stellar conditions across a large mass range

P. Nazari, J. D. Meijerhof, M. L. van Gelder +10

No statistical study of COMs toward a large sample of high-mass protostars with ALMA has been carried out so far. We aim to study six N-bearing species: CHCN, HNCO, NHCHO,…

astro-ph.SR2022★ 26 cited

Importance of source structure on complex organics emission II. Can disks explain lack of methanol emission from some low-mass protostars?

P. Nazari, B. Tabone, G. P. Rosotti +3

Some protostellar systems show little or no millimetre line emission of complex organics. This can be interpreted as a low abundance of these molecules, alternatively they could be…

astro-ph.SR2022★ 28 cited

Importance of source structure on complex organics emission. I. Observations of CHOH from low-mass to high-mass protostars

M. L. van Gelder, P. Nazari, B. Tabone +9

Complex organic molecules (COMs) are often observed toward embedded Class 0 and I protostars. However, not all Class 0 and I protostars exhibit COMs emission. In this work, variati…