  Using recent supernova models, I revisit the Supernova 1987a constraints on
scalar/pseudoscalar Axion-Like-Particles (ALPs). On the basis of the neutrino
detections, the luminosity of ALPs must be $\lesssim 5\times10^{52}
\,\mathrm{erg}/s$ after the core-bounce, and this bound limits ALPs couplings.
Contrary to the QCD axion models where all couplings are $\sim 1/f_a$, it has
been shown recently that a radion/dilaton could have far different coupling
strength to photons and to nucleons. This fact has raised a need to establish
the limits on each coupling independently. The bounds from ALPs emission by
nucleon-nucleon bremsstrahlung through a two-nucleon coupling and by the
Primakoff process through a two-photon coupling are updated considering the
total volume emission. I find the bounds on the two-photon coupling from the
Primakoff process differ from previous bounds by an order of magnitude. Through
the volume emission study, trapping regimes for $m_a\gtrsim10\,\mathrm{MeV}$
are also alleviated, which need to be probed by future experiments.
