首页> 外文会议>International Astronomical Union >3D Photoionisation Modelling of NGC 6302
【24h】

3D Photoionisation Modelling of NGC 6302

机译:NGC 6302的3D光激酶建模

获取原文

摘要

We present the first results from our 3D photoionisation modelling of NGC 6302, an extreme high-excitation bipolar planetary nebula with a dense dusty circumstellai disc. We are attempting to fully match the observed spectrum, including the high-ionization infrared coronal lines as well as the observed ISO spectrum. We use a bipolar model nebula with a dense circumstellar torus Our initial results show that, considering the very high stellar temperature required to match the high ionization coronal lines, an extremely high density contrast between the bipolar lobes and the circumstellar disc is required to match the nebular line ratios.
机译:我们通过NGC 6302的3D光激酶建模介绍了第一个结果,这是一个极端的高励磁双极行星星云,带有密集的尘土飞扬的Scretellai圆盘。我们正在尝试与观察到的光谱完全匹配,包括高电离红外冠状线以及观察到的ISO光谱。我们使用致密的星云与致密的星云,我们的初始结果表明,考虑到匹配高电阻冠线所需的非常高的恒星温度,双极裂片和外观盘之间的极高密度对比需要匹配地骨线比率。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
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