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BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20170622T103000
DTEND;TZID=Atlantic/Canary:20170622T113000
UID:iactalks-1060
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/1060
CREATED:2017-06-22T10:30:00+01:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:Mapping the Milky Way outer disk with LAMOST
DESCRIPTION:Mapping the Milky Way outer disk with LAMOST\nDr. Haifeng Wang\
 n\nBased on radial profiles, disk can be divided into three categories:Typ
 e I, classical single exponential (10%); Type II, down-bending joint expon
 ential (60%); Type III, up-bending joint exponential (30%). Milky Way is t
 he benchmark for the research of the disk Galaxy formation and evolution! 
 And the outer disks of galaxies present a unique laboratory for studying t
 he process of disk formation and it can provide us with a direct view of d
 isk assembly in progress. I will introduce my recent work about the milky 
 way outer disk. And some highlights about our group works with LAMOST data
  will also be mentioned.
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