N-body simulations show Galactic tides have not altered the outer stellar profiles of Sculptor and Ursa Minor, implying their extended stars are intrinsic rather than tidally stripped.
d d ]6I<z۟CSݝ :Zu#j4 ܞR iK N Vs5V 5A =s S=HmN ϛΥ 8<SϹm t ɪ _ɵ K芋z hؤ=H ]H 0NG] :vYtGd U8m2U ȝ- и bj gEw`AZA ym '
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
ACCEPT 1representative citing papers
citing papers explorer
-
Galactic tides and the outer density profile of the Sculptor and Ursa Minor dwarf spheroidals
N-body simulations show Galactic tides have not altered the outer stellar profiles of Sculptor and Ursa Minor, implying their extended stars are intrinsic rather than tidally stripped.