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SUMMARY:The masses of Local Group galaxies and the baryonic Tully-Fisher r
 elation
DTSTART;VALUE=DATE-TIME:20230320T113000Z
DTEND;VALUE=DATE-TIME:20230320T114500Z
DTSTAMP;VALUE=DATE-TIME:20241114T092409Z
UID:indico-contribution-222@meetings.aip.de
DESCRIPTION:Speakers: Stacy McGaugh (Case Western Reserve University)\nThe
  baryonic Tully-Fisher relation is a correlation between the quantity of s
 tars and gas in a galaxy and its flat rotation speed. The relation found i
 n external galaxies appears to hold for rotationally supported Local Group
  galaxies. It may also hold for some if not all of the pressure supported 
 dwarfs. The flat rotation speed depends on dynamical mass\, providing a co
 nstraint on total mass that is independent of other considerations.\n\nhtt
 ps://iaus379.aip.de/event/20/contributions/222/
LOCATION:Haus H\, Telegrafenberg
URL:https://iaus379.aip.de/event/20/contributions/222/
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