log(<i>gf</i>) values for astrophysically important transitions in Fe II /
| dc.campus | Chennai | |
| dc.contributor.author | Deb, Narayan C. | |
| dc.date.accessioned | 2025-02-20T08:40:33Z | |
| dc.date.accessioned | 2025-03-31T10:51:22Z | |
| dc.date.available | 2025-02-20T08:40:33Z | |
| dc.date.issued | 2012-11-05 | |
| dc.description.abstract | Recently Meléndez & Barbuy [1] reported accurate log(gf) values for 142 important astrophysical lines within the 4000Å to 8000Å wavelength range. We compare these log(gf) values with our calculated values in a large scale CI calculation involving the lowest 262 fine structure levels of Fe II. | |
| dc.identifier.uri | https://doi.org/10.1088/1742-6596/388/15/152005 | |
| dc.identifier.uri | https://dspacenew8-imu.refread.com/handle/123456789/2219 | |
| dc.language.iso | en | |
| dc.publisher | IOP Publishing | |
| dc.school | Others | |
| dc.title | log(<i>gf</i>) values for astrophysically important transitions in Fe II / | |
| dc.type | Article |
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