A DIFFICULTY WITH NE²² AS THE NEUTRON SOURCE FOR THE SOLAR SYSTEM S-PROCESSDESPAIN KH.1980; ASTROPHYS. J.; USA; DA. 1980; VOL. 236; NO 3 PART. 2; PP. L165-L168; BIBL. 19 REF.Article

ON THE MAXIMUM EXTENT OF FLASH-DRIVEN CONVECTION. II: THE CORE FLASHDESPAIN KH.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 253; NO 2; PART. 1; PP. 811-815; BIBL. 36 REF.Article

FLUORINE POWER AND HELIUM-SHELL FLASHES.SCALO JM; DESPAIN KH.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 203; NO 3 PART. 1; PP. 667-673; BIBL. 15 REF.Article

AN INTERPRETATION OF THE PUZZLING OBSERVATIONS OF FG SAGITTAE.CHRISTY SACKMANN IJ; DESPAIN KH.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 189; NO 3 PART. 1; PP. 523-530; BIBL. 27 REF.Article

CARBON AND ERUPTIVE STARS: SURFACE ENRICHMENT OF LITHIUM, CARBON, NITROGEN, AND ¹³C BY DEEP MIXING.SACKMANN IJ; SMITH RL; DESPAIN KH et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 187; NO 3 PART. 1; PP. 555-574; BIBL. 46 REF.Article