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: | , , |
|---|---|
| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
IOP Publishing
2015
|
| Online Access: | http://hdl.handle.net/1721.1/94540 https://orcid.org/0000-0001-9085-3821 |