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T. Contini

23 papers hereh-index 7623.3k citations509 works total

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

author position
  • sole author2
  • first author3
  • middle author8
  • last author3

Across the 16 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph23
same name
  • T. Contini — 1 paper
  • T. Contini — 1 paper, h 6

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
19952006
most citedRadiodetection of Cosmic Ray Extensive Air Showers

8 citations · 8 across the 7 of their papers we have counts for

collaborators
Showing 1999Show all

4 papers · 1 filter

astro-ph1999

The Chemical Evolution of Galaxies by Successive Starbursts

T. Contini, R. Coziol, S. Considere +2

We propose an evolutionary scenario by successive bursts of star formation to reproduce the chemical properties of massive nearby Starburst Nucleus Galaxies (SBNGs). The N/O abunda…

astro-ph1999

Infrared line ratios revealing starburst conditions in galaxies

Sueli M. Viegas, Marcella Contini, Thierry Contini

The physical conditions in typical starburst galaxies are investigated through critical infrared (IR) line ratios, as previously suggested by Lutz et al. (1998, A&A, 333, L75). The…

astro-ph1999

The abundance of nitrogen in starburst nucleus galaxies

R. Coziol, R. E. Carlos Reyes, S. Considere +2

We show that the excess of nitrogen emission observed in a large sample of Starburst Nucleus Galaxies (SBNGs) can only be explained at a given metallicity by an overabundance of ni…

astro-ph1999

Starbursts in barred spiral galaxies. V. Morphological analysis of bars

S. Chapelon, T. Contini, E. Davoust

We have measured the bar lengths and widths of 125 barred galaxies observed with CCDs. The dependence of bar strength (identified with bar axis ratio) on morphological type, nuclea…

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