A Runaway Yellow Supergiant Star in the Small Magellanic Cloud
Kathryn Neugent, Philip Massey, Nidia Morrell, Brian Skiff, and Cyril, Georgy

TL;DR
This paper reports the discovery of the first known runaway yellow supergiant star in the Small Magellanic Cloud, providing insights into stellar dynamics and galaxy evolution.
Contribution
It presents the identification and analysis of the first evolved runaway star outside the Milky Way, highlighting its properties and potential origin from a supernova explosion in a binary system.
Findings
First runaway yellow supergiant discovered outside the Milky Way.
Star's properties consistent with a 30 million-year-old, 9 solar mass star.
Star could have traveled 1.6 degrees across the SMC in 10 million years.
Abstract
We recently discovered a yellow supergiant (YSG) in the Small Magellanic Cloud (SMC) with a heliocentric radial velocity of ~300 km/s which is much larger than expected for a star in its location in the SMC. This is the first runaway YSG ever discovered and only the second evolved runaway star discovered in a different galaxy than the Milky Way. We classify the star as G5-8I, and use de-reddened broad-band colors with model atmospheres to determine an effective temperature of 4700+/-250K, consistent with what is expected from its spectral type. The star's luminosity is then L/Lo ~ 4.2+/-0.1, consistent with it being a ~30Myr 9Mo star according to the Geneva evolution models. The star is currently located in the outer portion of the SMC's body, but if the star's transverse peculiar velocity is similar to its peculiar radial velocity, in 10Myr the star would have moved 1.6 degrees across…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research
