Communications Presentées Au ... Colloque International D'astrophysique
But ^hey lie below the main sequence in the U-B, B-V diagram by up to 0.2 ( Jaschek and Jaschek 1957, 1959) as well ... line that is weaker in Am than in normal stars with the same hydrogen line type, is earlier than the UV type (van Dijk et al.
| Title | : | Communications Presentées Au ... Colloque International D'astrophysique |
| Author | : | |
| Publisher | : | - 1981 |
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