POSSIBLE EXPLANATION FOR ORIGIN OF LITHIUM, BERYLLIUM, AND BORON

[1] Bethe H, 1930, ANN PHYS-BERLIN, V5, P325

[2] BODANSKY D, 1972, PRIVATE COMMUNICATIO

[3] LITHIUM AND S-PROCESS IN RED-GIANT STARS [J]. ASTROPHYSICAL JOURNAL, 1971, 164 (01) : 111 - &

[4] CAMERON AGW, IN PRESS

[5] 327-MHZ OBSERVATIONS OF GALACTIC CENTER - POSSIBLE DETECTION OF A DEUTERIUM ABSORPTION LINE [J]. ASTROPHYSICAL JOURNAL, 1973, 180 (01) : L1 - L6

[6] CESARSKY DA, IN PRESS

[7] COLGATE SA, 1973, PREPRINT

[8] FOWLER WA, 1955, ASTROPHYS J S, V2, P167

[9] ORIGIN OF DEUTERIUM [J]. NATURE, 1973, 241 (5389) : 384 - 386

[10] DEUTERIUM IN ORION NEBULA [J]. ASTROPHYSICAL JOURNAL, 1973, 179 (02) : L57 - L59

[1] Bethe H, 1930, ANN PHYS-BERLIN, V5, P325

[2] BODANSKY D, 1972, PRIVATE COMMUNICATIO

[3] LITHIUM AND S-PROCESS IN RED-GIANT STARS [J]. ASTROPHYSICAL JOURNAL, 1971, 164 (01) : 111 - &

[4] CAMERON AGW, IN PRESS

[5] 327-MHZ OBSERVATIONS OF GALACTIC CENTER - POSSIBLE DETECTION OF A DEUTERIUM ABSORPTION LINE [J]. ASTROPHYSICAL JOURNAL, 1973, 180 (01) : L1 - L6

[6] CESARSKY DA, IN PRESS

[7] COLGATE SA, 1973, PREPRINT

[8] FOWLER WA, 1955, ASTROPHYS J S, V2, P167

[9] ORIGIN OF DEUTERIUM [J]. NATURE, 1973, 241 (5389) : 384 - 386

[10] DEUTERIUM IN ORION NEBULA [J]. ASTROPHYSICAL JOURNAL, 1973, 179 (02) : L57 - L59