taken from 2 paper(s):
/T.L.Bosler et al.(2007)/ /M.Gullieuszik et al.(2009)/
T.L.Bosler et al.,MNRAS, 378, 318, 2007(ADS)
The chemical abundances of the stellar populations in the Leo I and II dSph galaxies
Chemical Abundances
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| Ca | N/A | -1.79+-0.15 | ... | ... | -1.77+-0.15 | 0.01+-0.15 | 4.57+-0.15 | Ca |
| Fe | N/A | -1.78+-0.16 | ... | ... | -1.78+-0.16 | ... | 5.72+-0.16 | Fe |
Binary Parameters
| Vrad | 286.4 |
Position
| Right Ascension : 10 08 30.97 | Declination : +12 16 40.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2002-02-08 | N/A | KECKLRIS | 14000 | 27 | 3600 | 286.4 |
M.Gullieuszik et al.,AAP, 500, 735, 2009(ADS)
New constraints on the chemical evolution of the dwarf spheroidal galaxy Leo I from VLT spectroscopy
Stellar Parameters
Chemical Abundances
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| Fe | N/A | -1.97 | ... | ... | -1.97 | ... | 5.53 | Fe |
Position
| Right Ascension : 10 08 31.00 | Declination : +12 16 40.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| N/A | N/A | VLTFORS2 | N/A | 58 | N/A | 282.4 |