There is a broad astrophysics research program at TRIUMF.  I will 
discuss three current experiments.  The first experiment is a 
measurement of the lifetime of the 6.791 MeV excited state of 15O 
using the transfer reaction 16O(3He,4He)15O in inverse kinematics at 
ISAC-II.  This state makes a large contribution to the radiative 
capture 14N(p,g)15O, which is the limiting rate in the CNO cycle at 
stellar temperatures.  The second study is a measurement of 3He-4He 
radiative capture at several relative energies from 1.5 to 2.8 MeV 
using the DRAGON recoil mass spectrometer at ISAC-I, which has 
implications for the astrophysical factor S34 and the cosmological 7Li 
abundance.  The third experiment is an elastic scattering measurement 
using a radioactive beam of 8Li on 12C at ISAC-II with the TUDA 
facility.  The goal of this experiment is to limit the dominant 
systematic uncertainty in the value of the low energy cross section of 
7Be(p,gamma)8B  inferred from asymptotic normalization coefficient 
determinations in transfer reactions.