Marisa Girardi homepage

• Email: girardi at oats.inaf.it
• Phone: (+39) 040-3199-147
• Fax: (434) 040-3199-123
• Office Hours: 11:00 a.m. - 1:00 p.m.
• Office: 238 Villa Bazzoni - 1st floor
• Address:

  Department of Physics - Astronomy Unit
  University of Trieste
  11, Via Tiepolo
  34143 Trieste (TS)
  Italy

Galaxy cluster Abell 520

Multiwavelength image of the radio-halo galaxy cluster Abell 520 (coverpage of A&A, Vol. 491, Girardi et al. 2008).

Research Interests:

• Clusters of galaxies
• Clusters: mass and internal dynamics
• Clusters with radio halos/relics
• Groups of Galaxies
• Galaxies and environmental effects
• Galaxy evolution
• Observational cosmology

Projects and Available Grants:

• DARC (Dynamical Analysis of Radio Clusters), based on TNG-Canary Islands data, PI M.Girardi.
• PRIN-INAF2010 Architecture and Tomography of Galaxy Clusters, PI M.Nonino within the CLASH/VIMOS project based on European Southern Observatory Large Programme P186.A-0798 (PI P. Rosati).
  • NEW!!! two-years fellowship.
• FOGO (Origin of Fossil Groups), based on ITP - Canary Islands Telescopes, PI A.Aguerri, 1st FOGO paper.
  

Curriculum Vitae:

• Degree, Physics, University of Trieste, 1988.
• Ph.D., Astrophysics, SISSA, 1992.
  
  Presently:
• Ricercatore - with tenures tracks since 2001 University of Trieste.
  
  More Informtion:
• Complete CV and Publication List as an Acrobat PDF file.
  • Last Modified: May 10, 2011
  
  
• Up-to-dated Publication List as an ADS
• see also Trieste Univ. webpage

Teaching at Trieste:

Sistemi autogravitanti (Laurea Specialistica in Astrofisica e Cosmologia) dal 2009/10, Moodle page.
Fisica I dal 2001 al 2010 (Meccanica e Termodinamica per le lauree di Sc.Ambientali e Chimica, Moodle Page.

Tesi disponibili, argomenti:

• Dinamica Interna dell'ammasso DARC Abell 1995.
• Dinamica Interna dell'ammasso DARC Abell 1351.
• Equipartizione di energia per unita' di massa fra gas ICM e galassie: il problema dei gruppi di galassie.
• Sottostrutture in ammassi di galassie.
• Confronto fra gli ammassi MKW e i gruppi fossili.
• Anistropia di velocita' orbitali per le galassie d'ammasso.
• Ammassi in fase di merging: cfr. con simulazioni.
• Stima di massa per i superammsi: cfr. con simulazioni.