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Published byAmie Lynch Modified over 9 years ago
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LOGO The Chemical and Color Evolution of M33 2008.12 Reporter: Jun Yin (Shao) Supervisor: Jinliang Hou (Shao)
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Contents Observations 1 Models 2 Results & Forming History 3 Summary 4
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Observation Sc II-III, i=56, D=840 kpc M tot =5~8×10 9 M ⊙ r d,tot =2.4kpc, r d,* ~1.4kpc no merger whole gas & SFR abundance SB, color
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Observation H 2,tot =0.2×10 9 M ⊙, HI tot =2.2×10 9 M ⊙ r d,H2 =2.5kpc, r d,tot =7.8kpc whole gas & SFR abundance SB, color
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Observation whole gas & SFR abundance SB, color
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Observation Munoz-Mateos et al. (2007) M FUV = -16.63 (GALEX) M K = -21.78 (2MASS) whole gas & SFR abundance SB, color
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Chemical & Color Evolution Model Star Formation Rate Gas Infall Rate Outflow…… mass SFR Z, MDF color …… stellar evolution theoryInitial conditions
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Model f out ~b·Ψ, Z out =Z(t) Ψ~(Σ gas ) 1.4 r -1 f in ~t·exp(-t/τ), Z in =0 t d =a·r Gyr M tot =7×10 9 M ⊙, r d,tot =2.2kpc Σ tot (r)=230*exp(-r/r d,tot ) Total SFR Infall rate Outflow
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Results & Forming History Does M33 form quickly ? if τsmall infall quick gas , SFR low stellar disk big abundance high, steep SB dark, color red NO τ= r+5 Gyr
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Results & Forming History Does infall delay at outer part ? if t d large infall late gas fraction high stellar disk small abundance low, steep color blue, steep Not necessary t d = 0 Gyr -0.015 -0.022 -0.034 μ r = 23.2 mag arcsec -2 G kpc = -0.016
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Results & Forming History Does gas flow out ? if b large outflow large gas, SFR, star do not change much abundance low, flat color a little flatter YES ! b=1.0 -0.020 -0.017 -0.015 μ r = 23.2 mag arcsec -2 G kpc = -0.016
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Results & Forming History MDF & evolution of some global variables in our best model τ= r+5 Gyr t d = 0 Gyr b= 1.0
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Summary M33 should be forming though slow accretion process, i.e. longer infall time scale. The whole disk should form simutaneously, no obvious infall delay at outer disk. Outflow is not negligible because of its low metallicity. The M33 should obey similar SF law with our Galaxy.
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LOGO
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