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Radio astronomy techniques : the use of radio instruments from single dish radio telescopes to radio interferometers

机译:射电天文技术:从单碟射电望远镜到无线电干涉仪的无线电仪器的使用

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摘要

New radio telescopes under development, will significantly enhance the capabilitiesof radio astronomy in the Southern Hemisphere. South Africa, inparticular, is actively involved in the development of a new array (MeerKAT)as well as in the expansion of existing very long baseline interferometer arraysin the south. Participation in these new developments demands a thoroughunderstanding of radio astronomy techniques, and data analysis, and thisthesis focusses on two projects with the aim of gaining such experience.The Southern Hemisphere very long baselines array is not well servedwith calibrator sources and there are significant gaps in the present calibratordistribution on the sky. An adequately dense, well distributed, set of strong,compact calibrator or reference sources is needed. With this in mind, observationsusing the Southern Hemisphere long baseline array were conducted toinvestigate a sample of candidate calibrator sources. The compactness of thesources was investigated and new potential calibrators have been identified.Single antenna radio spectroscopy of OH masers has identified sourcesof 1720 MHz emission associated with supernova remnants at the shock interfacebetween the expanding supernova remnant and a molecular cloud.Models indicate that these masers are shock excited and can only be producedunder tight physical constraints. Outows from newly-formed starscreate nebulous regions known as Herbig-Haro objects when they interactwith the surrounding medium, and these regions are potentially similar tothose seen in supernova remnants. If conditions behind the shock fronts ofHerbig-Haro objects are able to support 1720-MHz OH masers they couldbe a useful diagnostic tool for star formation. A survey toward Herbig-Haroobjects using a single-dish radio telescope did detect 1720-MHz OH lines inemission, but neither their spectral signature nor follow-up observations withthe Very Large Array showed evidence of maser emission.
机译:正在开发的新型射电望远镜将大大增强南半球射电天文的能力。尤其是南非,积极参与开发新的阵列(MeerKAT)以及扩展南部现有的非常长的基线干涉仪阵列。参与这些新发展需要对射电天文学技术和数据分析有透彻的了解,并且本文着重于两个项目,目的是获得此类经验。南半球非常长的基线阵列不能很好地与校准源配合使用,并且在当前校准器在天空中的分布。需要足够密集,分布均匀的一组坚固紧凑的校准器或参考源。考虑到这一点,使用南半球长基线阵列进行了观测,以调查候选校准物来源的样本。 OH masers的单天线无线电波谱已经确定了与超新星残余物有关的1720 MHz发射源,该信号与正在膨胀的超新星残余物和分子云之间的冲击界面有关。模型表明,这些masers是激振,只能在严格的物理约束下产生。当新形成的恒星与周围的介质相互作用时,它们的出射流形成了一个名为Hertig-Haro的星云状区域,这些区域可能与超新星遗留物相似。如果Herbig-Haro物体的冲击波前沿后面的条件能够支持1720 MHz的OH脉冲,则它们可能是形成恒星的有用诊断工具。使用单碟射电望远镜对Herbig-Haroobject进行的一项调查确实检测到1720 MHz OH线的发射,但是它们的光谱特征和超大型阵列的后续观察都没有显示出大量发射的证据。

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    De Witt Aletha;

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  • 年度 2012
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