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Chinese Academy of Sciences Institutional Repositories Grid
A HIGH-VELOCITY BULGE RR LYRAE VARIABLE ON A HALO-LIKE ORBIT

文献类型:期刊论文

作者Kunder, Andrea1; Rich, R. M.2; Hawkins, K.3; Poleski, R.4,5; Storm, J.1; Johnson, C. I.6; Shen, J.7; Li, Z. -Y.7; Cordero, M. J.8; Nataf, D. M.9
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2015-07-20
卷号808期号:1页码:1
关键词Galaxy: bulge Galaxy: formation Galaxy: halo Galaxy: kinematics and dynamics stars: Population II stars: variables: RR Lyrae
英文摘要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, which has the unusual radial velocity of -372 +/- 8 km s(-1) and true space velocity of -482 +/- 22 km s(-1) 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.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]RED CLUMP STARS ; GALACTIC BULGE ; LIGHT CURVES ; BAADE WINDOW ; OGLE-III ; GALAXY ; METALLICITY ; EXTINCTION ; MAGNITUDE ; DISTANCE
收录类别SCI
语种英语
WOS记录号WOS:000358778900012
源URL[http://119.78.226.72/handle/331011/28215]  
专题上海天文台_星系宇宙学重点实验室
作者单位1.Leibniz Inst Astrophys Potsdam AIP, D-14482 Potsdam, Germany
2.Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
3.Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
4.Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
5.Univ Warsaw Observ, PL-00478 Warsaw, Poland
6.Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
7.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
8.Zentrum Astron, Astron Rech Inst, D-69120 Heidelberg, Germany
9.Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia
10.Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy
推荐引用方式
GB/T 7714
Kunder, Andrea,Rich, R. M.,Hawkins, K.,et al. A HIGH-VELOCITY BULGE RR LYRAE VARIABLE ON A HALO-LIKE ORBIT[J]. ASTROPHYSICAL JOURNAL LETTERS,2015,808(1):1.
APA Kunder, Andrea.,Rich, R. M..,Hawkins, K..,Poleski, R..,Storm, J..,...&Mroz, P..(2015).A HIGH-VELOCITY BULGE RR LYRAE VARIABLE ON A HALO-LIKE ORBIT.ASTROPHYSICAL JOURNAL LETTERS,808(1),1.
MLA Kunder, Andrea,et al."A HIGH-VELOCITY BULGE RR LYRAE VARIABLE ON A HALO-LIKE ORBIT".ASTROPHYSICAL JOURNAL LETTERS 808.1(2015):1.

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