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首页> 外文期刊>The Astrophysical Journal. Supplement Series >A Wide-Area VLA Continuum Survey near the Galactic Center at 6 and 20 cm Wavelengths
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A Wide-Area VLA Continuum Survey near the Galactic Center at 6 and 20 cm Wavelengths

机译:银河中心附近的广域VLA连续谱调查,波长为6和20 cm

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摘要

We describe the results of a millijansky sensitivity VLA survey of roughly 1 deg2 near the Galactic center at 6 and 20 cm. Catalogs of compact and filamentary structures are given and compared to previous surveys of the region. Eight of the unusual nonthermal radio filaments are detected in 6 cm polarized emission; three of these are the first such detections, confirming their nonthermal nature. This survey found emission from a filament at , or a projected distance from Sgr A* of 200 pc, greatly extending the latitude range observed with such features. There is also new evidence for spatial gradients in the 6/20 cm spectral indices of some filaments, and we discuss models for these gradients. In studying compact sources, the combination of spectral index and polarization information allows us to identify pulsar candidates and compact H ii regions in the survey. There is also some evidence that the flux measurements of compact sources may be affected by electron scattering from the interstellar medium in the central few hundred parsecs of the Galaxy.
机译:我们描述了在6和20厘米银河中心附近大约1度2的millijansky灵敏度VLA调查的结果。给出了致密和丝状结构的目录,并与该地区以前的调查进行了比较。在6 cm的极化发射中检测到八根异常的非热辐射灯丝;其中三个是首次此类检测,确认了它们的非热性质。这项调查发现,在200 pc的Sgr A *或距Sgr A *的预计距离处有细丝发射,大大扩展了使用此类功能观察到的纬度范围。还有一些新证据表明某些细丝的6/20 cm光谱指数存在空间梯度,我们讨论了这些梯度的模型。在研究紧凑型源时,光谱指数和极化信息的结合使我们能够确定脉冲星候选者和调查中的紧凑型H ii区域。还有一些证据表明,紧凑源的通量测量可能会受到银河系中央几百秒差距中来自星际介质的电子散射的影响。

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