20-24 March 2023
Haus H, Telegrafenberg
Europe/Berlin timezone

The masses of Local Group galaxies and the baryonic Tully-Fisher relation

20 Mar 2023, 12:30
15m
Haus H, Telegrafenberg

Haus H, Telegrafenberg

Potsdam, Germany
Contributed talk SESSION 1: From ground and space: motions, distances, chemistry and star formation measurements SESSION 1: From ground and space: motions, distances, chemistry and star formation measurements

Speaker

Stacy McGaugh (Case Western Reserve University)

Description

The baryonic Tully-Fisher relation is a correlation between the quantity of stars and gas in a galaxy and its flat rotation speed. The relation found in 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 constraint on total mass that is independent of other considerations.

Do you plan to attend the symposium in-person or virtually? in-person

Primary author

Stacy McGaugh (Case Western Reserve University)

Presentation Materials