A halo blue straggler on a highly eccentric retrograde orbit
A. Tillich, N. Przybilla, R.-D. Scholz, U. Heber

TL;DR
This paper reports the discovery and analysis of a high-velocity, metal-poor blue straggler star on a highly eccentric retrograde orbit in the Galactic halo, shedding light on its origin and kinematics.
Contribution
It presents the first detailed spectral and kinematic analysis of a halo blue straggler star with an extreme retrograde orbit, highlighting its unique properties.
Findings
Star is a metal-poor halo blue straggler with [M/H]=-1.2.
Star exhibits a highly eccentric retrograde orbit in the Galaxy.
Star's velocity exceeds typical blue straggler speeds but remains bound to the Galaxy.
Abstract
Blue straggler, which are stars that appear to be younger than they should be, are an important population of unusual stars in both stellar clusters and the halo field of the Galaxy. Most formation scenarios evoke either stellar collisions or binary stars that transfer mass or merge. We investigate high-velocity stars in the Galactic halo and perform a spectral and kinematical analysis to shed light on their nature and origin. Here we report that SDSSJ130005.62+042201.6 (J1300+0422 for short) is an A-type star of unusually large radial velocity (504.6 5 \kms). From a quantitative NLTE (and LTE) spectral analysis of medium-resolution optical spectra, the elemental composition is derived. Proper motion measurements combined with a spectroscopic distance estimate allow us to determine its present space velocity. Its kinematical properties are derived by integrating the equation of…
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