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M. Tosi

35 papers hereh-index 426.1k citations283 works total

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

author position
  • sole author8
  • first author1
  • middle author6
  • last author7

Across the 22 of 35 papers where every author was matched, so the position is known.

fields
  • astro-ph34
  • astro-ph.GA1
same name
  • M. Tosi — 37 papers, h 40
  • M. Tosi — 6 papers, h 20
  • M. Tosi — 1 paper, h 3
  • M. Tosi — 1 paper
  • M. Tosi — 1 paper, h 113

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
19932009
most citedThe Stellar Mass Distribution in the Giant Star Forming Region NGC 346

77 citations · 350 across the 17 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

astro-ph2006★ 74 cited

Deuterium astration in the local disc and beyond

Donatella Romano, Monica Tosi, Cristina Chiappini +1

(Abridged) Estimates of the interstellar deuterium abundance span a wide range of values. Here we study the evolution of deuterium in the framework of successful models for the che…

astro-ph2006★ 37 cited

BVI photometry of the very old open cluster Berkeley 17

Angela Bragaglia, Monica Tosi, Gloria Andreuzzi +1

We have obtained BVI CCD imaging of Berkeley 17, an anticentre open cluster that competes with NGC 6791 as the oldest known open cluster. Using the synthetic colour magnitude diagr…

astro-ph2006★ 19 cited

The old anticentre open cluster Berkeley 32: membership and fundamental parameters

V. D'Orazi, A. Bragaglia, M. Tosi +2

We have obtained medium-low resolution spectroscopy and BVI CCD imaging of Berkeley 32, an old open cluster which lies in the anticentre direction. From the radial velocities of 48…

astro-ph2006

The metallicity of the old open cluster NGC 6791

Raffaele Gratton, Angela Bragaglia, Eugenio Carretta +1

We have observed four red clump stars in the very old and metal-rich open cluster NGC 6791 to derive its metallicity, using the high resolution spectrograph SARG mounted on the TNG…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.