Free Access
Table B.1
Overview of possible significant contamination from stellar lines to the interstellar line equivalent width measurements.
| Measured line | Contaminating line | Spectral types | Contamination W |
|
|
|||
| 5780 Å | Fe ii (5780.1 Å) | B5V-A0V | 13 mÅ |
| ′′ | <B5V | <4 mÅ | |
| He i (5780.5 Å) | O9V | ~2 mÅ | |
| 6379 Å | Ne ii (6379.6 Å) | B0V, B1V, B2V | 8, 22, 8 mÅ |
| CH (4300.3 Å) | Ti ii (4300.0 Å) | B5V | 4 mÅ |
| ′′ | A0V | 161 mÅ | |
| CH+ (4232.5 Å) | Fe ii (4232.8 Å) | B2V | <12 mÅ |
| ′′ | B5V | ~98 mÅ | |
| A0V | ~300 mÅ | ||
| Si ii (4233.2 Å) | B2V | <12 mÅ | |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.