| タイトル | The Homunculus: a Unique Astrophysical Laboratory |
| 本文（外部サイト） | http://hdl.handle.net/2060/20060052423 |
| 著者（英） | Nielsen, K. E.; Gull, T. R. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2006-08-01 |
| 言語 | eng |
| 内容記述 | eta Car is surrounded by bipolar shells, the Homunculus and the internal Little Homunculus, that are observed in both emission and absorption. Thin disks, located between the bipolar lobes, include the very bright Weigelt blobs and the neutral emission structure called the Strontium filament. All are affected by changes in UV and X-Ray flux of the binary system. For example, the normally ionized Little Homunculus recombines during the few month long spectroscopic minimum and then reionizes. Spectral data, obtained with Hubble Space Telescope/Space Telescope Imaging Spectrograph (HST/STIS) and with Very Large Telescope/UltraViolet Echelle Spectrograph (VLT/UVES), provide a wealth of information on spectroscopic properties of neutral and singly-ionized metals and on chemistry of nitrogen rich, carbon, oxygen poor, dense, warm gas. This information is important to understand gamma ray bursters (GRB) that reveal red-shifted near-UV metallic absorptions from pre-GRB stellar ejecta. |
| NASA分類 | Astrophysics |
| 権利 | Copyright, Distribution as joint owner in the copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/565082 |
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