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researcher

G. Sabatini

30 papers hereh-index 12281 citations40 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author7
  • middle author22
  • last author1

Across the 30 of 30 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA26
  • astro-ph.SR4
same name
  • G. Sabatini — 23 papers, h 5
  • G. Sabatini — 3 papers, h 2
  • G. Sabatini — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20172025
most citedThe ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). IX. Physical Properties and Spatial Distribution of Cores in IRDCs

68 citations · 347 across the 25 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.GA2019★ 26 cited

The 3D structure of CO depletion in high-mass prestellar regions

S. Bovino, S. Ferrada-Chamorro, A. Lupi +3

Disentangling the different stages of the star-formation process, in particular in the high-mass regime, is a challenge in astrophysics. Chemical clocks could help alleviating this…

astro-ph.GA2019

On the size of the CO-depletion radius in the IRDC G351.77-0.51

G. Sabatini, A. Giannetti, S. Bovino +5

An estimate of the degree of CO-depletion (fD​) provides information on the physical conditions occurring in the innermost and densest regions of molecular clouds. A key paramete…

astro-ph.GA2019★ 7 cited

Inquiring into the nature of the Abell 2667 Brightest Cluster Galaxy: physical properties from MUSE

E. Iani, G. Rodighiero, J. Fritz +21

Based on HST and MUSE data, we probe the stellar and gas properties (i.e. kinematics, stellar mass, star formation rate) of the radio-loud brightest cluster galaxy (BCG) located at…

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