Accepted –. Received – We present evidence for stochastic star formation histories in low-mass (M ∗ < 1010 M) galaxies from observations within the Galaxy And Mass Assembly (GAMA) sur-vey. For ∼73,000 galaxies between 0.05 < z < 0.32, we calculate star formation rates (SFR) and specific star formation rates (SSFR = SFR/M∗) from spectroscopic Hα
No takes yet. Share an insight, caveat, or question.
Bauer et al. (2013) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: