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26 April 2024 |
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Article overview
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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 | Abstract: | We 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 | Services: | Forum | Review | PDF | Favorites |
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