activity
20162026
most citedG11.92-0.61 MM1: A Keplerian disc around a massive young proto-O star

117 citations · 603 across the 30 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.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.GA2022★ 27 cited

Methanol deuteration in high-mass protostars

M. L. van Gelder, J. Jaspers, P. Nazari +6

The deuteration of molecules forming in the ices such as methanol (CHOH) is sensitive to the physical conditions during their formation in dense cold clouds and can be probed t…

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…