activity
19972004
collaborators

10 papers

astro-ph2004

A detailed study of the nuclear region of Mrk 273

M. Bondi, D. Dallacasa, M. A. Peerez Torres +1

We present 5 GHz EVN+MERLIN observations of the nuclear region of the ultra luminous infrared galaxy Mrk 273. These observations confirms the detection, on the mas scale, of two re…

astro-ph2004

The two sided parsec scale structure of the Low Luminosity Active Galactic Nucleus in NGC 4278

G. Giovannini, M. Giroletti, G. B. Taylor

We present new Very Long Baseline Interferometry observations of the LINER galaxy NGC 4278 with a linear resolution of < 0.1 pc. Our radio data reveal a two sided structure, with s…

astro-ph2004

Type II quasar candidates in the Sloan Digital Sky Survey: evidence for X-ray obscuration

C. Vignali, D. M. Alexander, A. Comastri

Recent X-ray surveys with Chandra and XMM-Newton have found several genuine Type II quasars, the long sought-after population of high-luminosity (high-redshift) Seyfert 2 galaxies,…

astro-ph2003

Variable stars as tracers of stellar populations in Local Group galaxies: Leo I and NGC 6822

L. Baldacci, F. Matonti, L. Rizzi +5

Results are presented of a study of the variable star populations in the dwarf spheroidal galaxy Leo I and in the dwarf irregular galaxy NGC 6822, based on time series photometry o…

astro-ph2003

Building up the Galactic Halo: The Sagittarius dSph and the globular cluster M22

L. Monaco, F. R. Ferraro, M. Bellazzini +1

The Sagittarius dwarf spheroidal (Sgr) and a few paculiar Galactic Globular Clusters (GGC) can be considered as building blocks of theGalactic Halo. We present a series of results…

astro-ph2000

Dynamic Work Distribution for PM Algorithm

E. Carretti, A. Messina

Although poor for small dynamic scales, the Particle-Mesh (PM) model allows in astrophysics good insight for large dynamic scales at low computational cost. Furthermore, it is poss…