The skeleton: connecting galaxy formation to large scale structures

Add to your list(s) Download to your calendar using vCal

• Christophe Pichon, Institut d'astrophysique de Paris/ Leverhulme visiting professor (Oxford)
• Thursday 18 November 2010, 16:30-17:30
• Sackler Lecture Theatre, IoA (tea at 4:00 pm).

If you have a question about this talk, please contact scott chapman.

I will report on morphological estimators of the filamentary structure of the Cosmic Web, the so-called skeleton. Based on a global study of the matter density gradient flow, it allows us to study the connectivity between a density peak and its surroundings, with direct relevance to the anisotropic accretion via cold flows on galactic halos. It also provides a theoretical framework to study their cosmic evolution through the onset of gravity-induced non-linearities. http://uk.arxiv.org/abs/0911.3779

This talk is part of the Institute of Astronomy Colloquia series.

This talk is included in these lists:

• Cambridge Astronomy Talks
• Combined External Astrophysics Talks DAMTP
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• Institute of Astronomy Colloquia
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
• Priscilla
• Sackler Lecture Theatre, IoA (tea at 4:00 pm)

Note that ex-directory lists are not shown.