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  • 标题:Perseus anomalous emission as seen with VSA
  • 本地全文:下载
  • 作者:R. Watson ; R. Rebolo ; R.D. Davies
  • 期刊名称:PoS - Proceedings of Science
  • 印刷版ISSN:1824-8039
  • 出版年度:2006
  • 出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
  • 摘要:We have observed the Perseus Molecular cloud at 33GHz at 7 arcminute resolution with the Very Small Array (VSA), which was previously identified as a strong source of anomalous dust correlated microwave emission at 1◦ with the COSMOSOMAS experiment. This emission represents a relatively new and poorly understood galactic foreground which may be significant at intermediate galactic latitudes. The angular resolution of the VSA makes it ideal for comparison with the IRAS satellite survey and is similar to that of the HFI channels of the forthcoming Planck mission. The morphology of this emission at 33 GHz consists of several 10 arcminute hot-spots coincident with the IRAS ‘knots’ in G159.6-18.5 plus a strange decrement, which is probably a hole in the diffuse anomalous component. We find the IRAS 25 mm data the most correlated template at 77% using the Pearson correlation statistic.
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