20 January 2012
Aula Grassano - Dipartimento di Fisica - Università degli Studi di Roma
Europe/Rome timezone

Session

Session - III : Astrophysics

20 Jan 2012, 14:20
Aula Grassano - Dipartimento di Fisica - Università degli Studi di Roma

Aula Grassano - Dipartimento di Fisica - Università degli Studi di Roma

Via della Ricerca Scientifica, 1 00133 Roma (ITALY)

Presentation materials

There are no materials yet.

  1. 20/01/2012, 14:20
    Classical Cepheids play a key role in constraining the astronomic distances. They are very bright variable stars, so they can be observed at great distances, and they obey to a well known Period Luminosity Relation (PL), so we can use the measured pulsation period and the observed magnitude to estimate the absolute magnitude. According to theoretical models the PL relation is expected to...
    Go to contribution page
  2. 20/01/2012, 14:40
    To ascertain the nature of celestial high energy sources, it is crucial to identify their optical counterparts. However, the currently available astronomical public optical databases do not provide an adequate support for a systematic high energy sources identification work. In particular, the optical limiting magnitude represents a severe limitation since the deepest flux limits reached by...
    Go to contribution page
  3. 20/01/2012, 15:00
    Galaxy clusters are the largest gravitationally bounded objects in the Universe. They are massive structures (M = 10^13 - 10^15 M_sun) containing tens to hundreds of galaxies interacting in a common potential well. Observations show that 10-20% of the total mass is made by hot (T=10^7-10^8 K) and diffuse ne= 10^(-4) - 10^(-2) cm^(-1) called IntraClusterMedium(ICM), emitting in the X-Ray band...
    Go to contribution page
  4. 20/01/2012, 15:30
  5. 20/01/2012, 15:50
    The Sun is an astrophysical source with a strong emission in the X-ray band. The study of solar flares is a key point for understanding the behaviour of the magnetic field of our star. In literature there are a lot of theories about polarization predictions, for a wide range of solar flares models but observations in the X-ray band have never been exhaustive. I will explore the possibility to...
    Go to contribution page
Building timetable...