PROBING THE "30 μm" FEATURE: LESSONS FROM EXTREME CARBON STARS
Some carbon-rich evolved stars exhibit a very prominent spectral feature at ~"30 μm." The C-rich nature of these objects suggests that the carrier is a sulfide, carbide, or other substance apt to form in a reducing environment. However, the carrier of this spectral feature remains disputed...
| Main Authors: | , , |
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing,
2015-02-17T13:59:57Z.
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| Subjects: | |
| Online Access: | Get fulltext |