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D. Bettoni

55 papers hereh-index 191.2k citations32 works total

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

author position
  • first author11
  • middle author28
  • last author5

Across the 44 of 55 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA20
  • astro-ph.CO19
  • astro-ph15
  • astro-ph.HE1
same name
  • D. Bettoni — 397 papers, h 51
  • D. Bettoni — 289 papers
  • D. Bettoni — 257 papers, h 29
  • D. Bettoni — 174 papers, h 46
  • D. Bettoni — 171 papers, h 5
  • D. Bettoni — 32 papers, h 4

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
20002025
most citedThe evolution of the galactic morphological types in clusters

315 citations · 2.8k across the 55 of their papers we have counts for

collaborators
Showing 2001Show all

4 papers · 1 filter

astro-ph2001★ 50 cited

The Fundamental Plane of Radio Galaxies

D. Bettoni, R. Falomo, G. Fasano +3

We collected photometrical and dynamical data for 73 low red-shift (z<0.2) Radio Galaxies (LzRG) in order to study their Fundamental Plane (FP). For 22 sources we also present new…

astro-ph2001★ 34 cited

The gas content of peculiar galaxies: counterrotators and polar rings

D. Bettoni, G. Galletta, S. Garcia-Burillo +1

This paper studies the global ISM content in a sample of 104 accreting galaxies, including counterrotators and polar rings, which spans the entire Hubble sequence. The molecular, a…

astro-ph2001★ 13 cited

The visible environment of galaxies with counterrotation

D. Bettoni, G. Galletta, F. Prada

In this paper we present a statistical study of the environments of 49 galaxies in which there is gas- or stellar- counterrotation. The number of possible companions in the field (…

astro-ph2001★ 57 cited

GRB010222: afterglow emission from a rapidly decelerating shock

N. Masetti

The GRB010222 optical and near-infrared (NIR) afterglow was monitored at the TNG and other Italian telescopes starting ~1 day after the high-energy prompt event. The optical BVR li…

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