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Stéphane Courteau

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Ascona/Terschelling Highlights<br />

• Most disk galaxies have additional, thick, disk<br />

(Yoachim/Dalcanton)<br />

– Modest mass fraction,<br />

but increases below<br />

v c~120 km s -1<br />

– Some counter-rotate:<br />

⇒ external origin<br />

– Heavier counter-rotating<br />

disks seen in S0s<br />

(Kannappan)<br />

• [α/Fe] vs [Fe/H] in MW thick disk ⇒ it cannot have<br />

formed by accretion of small stellar lumps (Venn)<br />

• Origin in gas-rich merger (Sommer-Larsen)

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