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Title: A Dynamically Distinct Stellar Population in the Leading Arm of the Sagittarius Stream
Abstract We present a chemical and dynamical analysis of the leading arm (LA) and trailing arm (TA) of the Sagittarius (Sgr) stream, as well as for the Sgr dwarf galaxy core (SC), using red giant branch, main-sequence, and RR Lyrae stars from large spectroscopic survey data. The different chemical properties among the LA, TA, and SC generally agree with recent studies and can be understood by a radial metallicity gradient established in the progenitor of the Sgr dwarf, followed by preferential stellar stripping from the outer part of the Sgr progenitor. One striking finding is a relatively larger fraction of low-eccentricity stars (e< 0.4) in the LA than in the TA and SC. The TA and SC exhibit very similar distributions. Considering that a tidal tail stripped off from a dwarf galaxy maintains the orbital properties of its progenitor, we expect that thee-distribution of the LA should be similar to that of the TA and SC. Thus, the disparate behavior of thee-distribution of the LA is of particular interest. Following the analysis of Vasiliev et al., we attempt to explain the differente-distribution by introducing a time-dependent perturbation of the Milky Way by the Large Magellanic Cloud's (LMC) gravitational pull, resulting in substantial evolution of the angular momentum of the LA stars to produce the low-estars. In addition, we confirm from RR Lyrae stars with high eccentricity (e> 0.6) that the TA stars farther away from the SC are also affected by disturbances from the LMC.  more » « less
Award ID(s):
1927130
PAR ID:
10543450
Author(s) / Creator(s):
; ; ;
Publisher / Repository:
APJL
Date Published:
Journal Name:
The Astrophysical Journal Letters
Volume:
954
Issue:
2
ISSN:
2041-8205
Page Range / eLocation ID:
L43
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
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