File:C26steranes-MS.gif
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Summary
| Description |
English: Because C26 steranes are generally present in a magnitude lower than other more common steranes (C27, C28, C29), GC/MS/MS is usually done in order to better analyze the C26 steranes. (a) shows the summation of GC/MS/MS transitions for all steranes whereas (b) shows transitions for only C26 steranes and where those peaks map to the summation. |
| Date | |
| Source | https://www.sciencedirect.com/science/article/pii/S0146638098001843#BIB28 |
| Author | A.G. Holba |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 05:56, 1 June 2019 | | 313 × 479 (16 KB) | Sarahhou2020 | User created page with UploadWizard |
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