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26 April 2024
 
  » arxiv » 1506.2664

 Article overview



A high-velocity bulge RR Lyrae variable on a halo-like orbit
Andrea Kunder ; R. Michael Rich ; Keith Hawkins ; Radek Poleski ; Jesper Storm ; Christian I. Johnson ; Juntai Shen ; Zhao-Yu Li ; Maria Jose Cordero ; David M. Nataf ; Giuseppe Bono ; Alistair R. Walker ; Andreas Koch ; Roberto De Propris ; Andrzej Udalski ; Michal K. Szymanski ; Igor Soszynski ; Grzegorz Pietrzynski ; Krzysztof Ulaczyk ; Lukasz Wyrzykowski ; Pawel Pietrukowicz ; Jan Skowron ; Szymon Kozlowski ; Przemyslaw Mroz ;
Date 8 Jun 2015
AbstractWe report on the RR Lyrae variable star, MACHO 176.18833.411, located toward the Galactic bulge and observed within the data from the ongoing Bulge RR Lyrae Radial Velocity Assay (BRAVA-RR), which has the unusual radial velocity of -372 +- 8 km/s and true space velocity of -482 +- 22 km/s relative to the Galactic rest frame. Located less than 1 kpc from the Galactic center and toward a field at (l,b)=(3,-2.5), this pulsating star has properties suggesting it belongs to the bulge RR Lyrae star population yet a velocity indicating it is abnormal, at least with respect to bulge giants and red clump stars. We show that this star is most likely a halo interloper and therefore suggest that halo contamination is not insignificant when studying metal-poor stars found within the bulge area, even for stars within 1 kpc of the Galactic center. We discuss the possibility that MACHO 176.18833.411 is on the extreme edge of the bulge RR Lyrae radial velocity distribution, and also consider a more exotic scenario in which it is a runaway star moving through the Galaxy.
Source arXiv, 1506.2664
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