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首页> 外文期刊>The Astrophysical journal >ABSOLUTE PROPER MOTION OF THE SAGITTARIUS DWARF GALAXY AND OF THE OUTER REGIONS OF THE MILKY WAY BULGE
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ABSOLUTE PROPER MOTION OF THE SAGITTARIUS DWARF GALAXY AND OF THE OUTER REGIONS OF THE MILKY WAY BULGE

机译:射手座矮人银河系和银河凸起外部区域的绝对正确运动

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摘要

We have determined the absolute proper motion of the Sagittarius dwarf spheroidal galaxy (Sgr) from the Southern Proper Motion Catalog 3, by selecting red giant candidates from the Two Micron All Sky Survey. We obtain μ_l cos b = -2.35 ± 0.20 and 蘝b = 2.07 ± 0.20 mas yr~(-1). Using the same procedure, we also determine the absolute proper motion of the bulge in the region of the sky that overlaps with Sgr. For the bulge, we obtain μ_l cos b = -5.86 ± 0.14 and μ_b = -0.59 ± 0.14 mas yr~(-1), at l = 7.6° and b = -21.2°. The absolute proper motions are on the International Celestial Reference System via Hipparcos Catalog stars.
机译:通过从“两次微米”全天候测量中选择红色巨人候选者,我们从南方适当运动目录3中确定了射手座矮球状星系(Sgr)的绝对正确运动。我们获得μ_lcos b = -2.35±0.20和蘝b = 2.07±0.20 mas yr〜(-1)。使用相同的步骤,我们还可以确定与Sgr重叠的天空区域中凸起的绝对正确运动。对于隆起,在l = 7.6°和b = -21.2°时,我们获得μ_lcos b = -5.86±0.14和μ_b= -0.59±0.14 mas yr〜(-1)。绝对正确的运动是通过Hipparcos目录星在国际天文参考系统上进行的。

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