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M. Capaccioli

4 papers here

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

author position
  • middle author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • M. Capaccioli — 3 papers
  • M. Capaccioli — 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

most citedIs there a dichotomy in the Dark Matter as well as in the Baryonic Matter properties of ellipticals?

1 citations · 1 across the 4 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2004

Galaxy dynamics with the Planetary Nebula Spectrograph

N. R. Napolitano, A. J. Romanowsky, N. G. Douglas +6

The Planetary Nebula Spectrograph is a dedicated instrument for measuring radial velocity of individual Planetary Nebulae (PNe) in galaxies. This new instrument is providing crucia…

astro-ph2003

Early-type Galaxy Halo Dynamics inferred using the PN Spectrograph

N. G. Douglas, A. J. Romanowsky, K. Kuijken +6

A new instrument is providing crucial data with which to probe the structure of dark halos in elliptical galaxies.

astro-ph2003★ 1 cited

Is there a dichotomy in the Dark Matter as well as in the Baryonic Matter properties of ellipticals?

N. R. Napolitano, M. Capaccioli, M. Arnaboldi +5

We have found a correlation betwen the M/L global gradients and the structural parameters of the luminous components of a sample of 19 early-type galaxies. Such a correlation suppo…

astro-ph2003

The cluster of galaxies A 2163B at z~0.2 II -- Colour gradients, re--mie relations and the Photometric Plane

F. La Barbera, G. Busarello, P. Merluzzi +3

This paper has been withdrawn by the author(s), since it has been merged with paper I (astro-ph/0307482).

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