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Observation and modelling of main-sequence star chromospheres – XVIII. Observations of the Ca ii resonance lines and Hα line for dM4 stars and dK5 stars†
Article first published online: 13 MAR 2012
DOI: 10.1111/j.1365-2966.2012.20649.x
© 2012 The Author Monthly Notices of the Royal Astronomical Society © 2012 RAS
Issue
Monthly Notices of the Royal Astronomical Society
Volume 421, Issue 4, pages 3189–3205, April 2012
Additional Information
How to Cite
Houdebine, E. R. (2012), Observation and modelling of main-sequence star chromospheres – XVIII. Observations of the Ca ii resonance lines and Hα line for dM4 stars and dK5 stars. Monthly Notices of the Royal Astronomical Society, 421: 3189–3205. doi: 10.1111/j.1365-2966.2012.20649.x
Publication History
- Issue published online: 10 APR 2012
- Article first published online: 13 MAR 2012
- Accepted 2012 January 30. Received 2012 January 29; in original form 2011 December 15
- Abstract
- Article
- References
- Supporting Information
- Cited By
Table 1. Some parameters of our dM4 stars.
Table 2. Some parameters of our dK5 stars.
Table 3. Equivalent widths measured for our dM4 stars.
Table 4. Equivalent widths measured for our dK5 stars.
Table 5. Our observations and observations compiled from the literature for our dM4 stars.
Table 6. Our observations and observations compiled from the literature for our dK5 stars.
| Filename | Format | Size | Description |
|---|---|---|---|
| MNR_20649_sm_tables1to6.zip | 13K | Supporting info item |
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