The Infrared Properties Of Local Mergers · The Merger catalogue • Blind Infrared Study • 3003...
Transcript of The Infrared Properties Of Local Mergers · The Merger catalogue • Blind Infrared Study • 3003...
Alfredo Carpineti, S. Kaviraj, D. L. Clements, D. Darg, A. K. Hyde, C. Lintott
The Infrared Properties Of
Local Mergers
The Merger catalogue
• Blind Infrared Study
• 3003 mergers from SDSS with z < 0.1 (Darg et al. 2010)
• Cross-matched with the IIFSCz(Wang & Rowan-Robinson 2009)
• 18% IRAS detected, 98% of which LTGs
• Poor IRAS resolution is an advantage
The UnDetected Mergers
• SFR(2*Ha) is a good approximation to SFRFIR
• From that we can extract an expected FIR flux
• Our IR detected mergers are the bright end of the bell curve
The Infrared properties
• Median Luminosity for IRAS-detected mergers is 1011 L⦿
• Median SFR (Kennicut et al.1998) 15 M⦿yr-1
SFR and Environments
• SFR independent of environment
• Environment density calculated using Schawinski et al. 2007
SFR and Mass/Mass Ratio
• SFR doesn’t depend on mass ratio but only on the total stellar mass of the system
Emission Line Activity
• AGN Fraction rises with L(IR)
• All the ULIRGs have AGN and are in a late merger state (c.f. Mirabel & Sanders 1996)
LIRG to ULIRG timescale
• How long does it take for a LIRG evolve?
• Morphological difference between LIRGs and ULIRGs
• All ULIRGs have core separation <5Kpc (4/10 already coalesced)
• 98% LIRGs have a core separation > 5Kpc
• Merger bias? ULIRGs from IIFSCz: 73% are post-mergers
LIRG to ULIRG timescale
• Newtonian approach -> how fast can a LIRG turn into a ULIRG?
• Median timescale 46 ± 16 Myr
Conclusions• 606 matches with the IIFSCz (18% GZ SDSS mergers)
• On average they have LIRG luminosity
• Prefer low density environment, SFR constant respect to environment
• SFR depends on the total mass, independent of mass ratio
• AGN fraction increases with L(FIR), agreement with LIRGs/ULIRGs studies
• LIRG to ULIRG timescale has a lower limit of 46 Myr
Conclusions
The average infrared bright merger is a minor spiral-spiral LIRG, which lives in a low density environment, has a moderate star-formation rate and possibly some form of AGN activity
Carpineti et al. (in preparation)