Now showing items 1-3 of 3

    • Tang, XD; Azhari, A.; Gagliardi, Carl A.; Mukhamedzhanov, AM; Pirlepesov, F.; Trache, L.; Tribble, Robert E.; Burjan, V.; Kroha, V.; Carstoiu, F. (American Physical Society, 2003)
      The evolution of very low-metallicity, massive stars depends critically on the amount of CNO nuclei that they produce. Alternative paths from the slow 3alpha process to produce CNO seed nuclei could change their fate. The ...
    • Tang, XD; Azhari, A.; Fu, CB; Gagliardi, Carl A.; Mukhamedzhanov, AM; Pirlepesov, F.; Trache, L.; Tribble, Robert E.; Burjan, V.; Kroha, V.; Carstoiu, F.; Irgaziev, BF. (American Physical Society, 2004)
      N-13(p, gamma)O-14 is one of the key reactions which trigger the onset of the hot CNO cycle. This transition occurs when the proton capture rate on 13N is faster, due to increasing stellar temperature (greater than or equal ...
    • Moretto, S.; Fabris, D.; Lunardon, M.; Pesente, S.; Rizzi, V.; Viesti, G.; Barbui, M.; Cinausero, M.; Fioretto, E.; Prete, G.; Brondi, A.; Vardaci, E.; Lucarelli, F.; Azhari, A.; Tang, XD; Hagel, K.; Ma, Y.; Makeev, A.; Murray, M.; Natowitz, J. B.; Qin, L.; Smith, P.; Trache, L.; Tribble, Robert E.; Wada, R.; Wang, J. (American Physical Society, 2004)
      Fusion-evaporation reactions induced by 110 MeV B-11 and radioactive C-11 on Rb-87 targets have been studied by measuring evaporation residue-light particle coincidences. The proton to alpha particle ratio in each reaction ...