...
首页> 外文期刊>The Astrophysical journal >Optically Thick Radio Cores of Narrow-Waist Bipolar Nebulae
【24h】

Optically Thick Radio Cores of Narrow-Waist Bipolar Nebulae

机译:窄腰双极星云的光学厚的无线电核心

获取原文

摘要

We report our search for optically thick radio cores in 16 narrow-waist bipolar nebulae. Optically thick cores are a characteristic signature of collimated ionized winds. Eleven northern nebulae were observed with the Very Large Array (VLA) at 1.3 and 0.7 cm, and five southern nebulae were observed with the Australia Telescope Compact Array (ATCA) at 6 and 3.6 cm. Two northern objects, 19W32 and M1-91, and three southern objects, He 2-25, He 2-84, and Mz 3, were found to exhibit a compact radio core with a rising spectrum consistent with an ionized jet. Such jets have been seen in M2-9 and may be responsible for shaping bipolar structure in planetary nebulae.
机译:我们报告了我们对16个窄腰双极星云中光学较厚的无线电核心的搜索。光学上较厚的磁芯是准直离子风的特征。在1.3和0.7厘米处的超大型阵列(VLA)观测到11个北部星云,在6和3.6 cm处的澳大利亚望远镜紧凑阵列(ATCA)观测到5个南部星云。发现两个北部天体19W32和M1-91,以及三个南部天体He 2-25,He 2-84和Mz 3表现出一个紧凑的无线电核心,其上升的频谱与电离射流一致。在M2-9中已经发现了这样的喷流,它们可能是在行星状星云中塑造双极结构的原因。

著录项

获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号