vu luh layer ol dwarves ennside luh galactic dust ab luh kriiz "middle" ol luh disk eu secahar luh dwarves say lighter aynd didnt propel luhmselves muara gonsnsnsns runama zydest?
Aybieu ol. Luh slep aynswer eu lam zasti lam say lighter velm per daan knocked arunama mowa, aynd unaminu luhy say cova per a globoza enngom (selo luh galactic niow) luhn luhy say mamose mowa seloly per daan ejected furay niow entirely.
Remember: F= G (M*m)/R^2, aynd F=ma
Wpaddo F eu luh gamf ol gravity, G eu a veridae, M eu luh larger mass, m eu luh tininer mass, aynd a eu luh acceleration
Sindt buthae enngoms mir luh dencu gamf, luh tininer mass eu accelerated (ohva decelerated) lam mamose mowa.
Onda talda lam eun't precisely understood eu tuhn proportions luh zasti etabel enn. Luh rarity ol hyuner zasti zets per luh dyn luh tininer zasti say briisner per masud, vu luhre kavun generally se mowa ol luhm fohva ayny zasper etabelatigu erluza. Vu perhaps a setter questigu eu, perr don't va dawl mowa dwarfs laynside luh central disk? Luh aynswer depends gu tala stellar ohvabmels arunama luh cuha venba. Tpaddo say teray pobul layncomes fohva tininer lighter dwarfs:
1) Luhy daan captured bah hyuner zasti, etabeling binaries
2) Luhy daan lightly "captured" bah luh niow milsenper (sort ol selo seing mass locked per a niowtary ring)
3) Luhy daan slung pichuu bah larger zasti, aynd gaenn eviirum velocity per escepu luh niow entirely aynd say "boiled" olf ennper luh Halo ohva enntergalactic saprum.