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Aday Robaina Rapisarda (Yes, two surnames)

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Presentation on theme: "Aday Robaina Rapisarda (Yes, two surnames)"— Presentation transcript:

1 Aday Robaina Rapisarda (Yes, two surnames)
Enhanced SFR in galaxy pairs and mergers from IR-bright galaxies in GEMS Aday Robaina Rapisarda (Yes, two surnames) Lago di Como, Italy

2 Looking for mergers (nothing to do with the talk title)
In the local universe, everybody agrees on their classifications. Random one Antennae M101

3 What about the far ones? Let’s say z>0.5

4 Automatic Classifiers: Concentration and Asymmetry
Early types (0<A<0.5) Late types (0.35<A<1.1)

5 Tested on close galaxy samples (Fried catalogue)
Strange guys A>0.7 Automated classifiers designed to imitate human eye Tested on close galaxy samples (Fried catalogue) Work reasonably well on isolated galaxies, but…

6 I don’t know and they don´t explain
What about this? I don’t know and they don´t explain

7 Enhanced Star Formation in Interactions
(Approaching the end of the talk) Local universe High redshift Lambas et al. 2003 Lin et al. 2006

8 GEMS Results New statistical approach (no need for 2-point correlation function) Clear enhancement in close pairs and mergers Averaged SFR in pairs defined Error bars minimized due to the new approach (not too bad compared with spectroscopic surveys) Results will improve with the STAGES dataset

9 Merger Fraction in 24μm Sample
Merger fraction clearly increases with TIR luminosity 20% TIR luminosity in strong mergers 30% TIR luminosity in interactions Mergers 2.09 times brighter than “normal” pairs Rapid decline in the CSFH is not due to a merger evolution (more restrictive results than in Bell et al. 2005)

10 Blue-Rose-Ring Galaxy
LIRG Starburst X-ray Spectacular Morphology


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