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| Description |
English: Probing the Last Gasps of Doomed Star Eta Carinae. The spectrum covers approximately 700nm - 760nm in the near infrared. The broard HeI line is from the primary wind, while the narrow forbidden ionised metal lines are from the surrounding nebula. The ArIII line may arise from the colliding wind zone.
Magyar: A frissen javított STIS által készített spektrum a pusztulófélben lévő Éta Carinae óriáscsillagról |
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| Date | (released) | ||
| Source | https://www.nasa.gov/mission_pages/hubble/multimedia/ero/ero_eta_carinae.html | ||
| Author | NASA, ESA, and the Hubble SM4 ERO Team | ||
| Permission (Reusing this file) |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 12:12, 20 June 2014 | | 1,600 × 1,200 (134 KB) | Regasterios | {{Information |Description ={{en|1=Probing the Last Gasps of Doomed Star Eta Carinae}} {{hu|1=A frissen javított STIS által készített spektrum a pusztulófélben lévő Éta Carinae óriáscsillagról}} |Source =http://www.nasa.gov/missi... |
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