CH₃OH spectra (  ×  ) toward the four positions identified in Fig. 1 in the Orion BN/KL region. The methanol rotational temperatures and column densities are estimated by a least-squares fit, where the uncertainties include the statistical error, the rms noise, and calibration uncertainties (10%). Blue dashed lines indicate the fits with fixed temperatures. Black dashed lines indicate a V_LSR of 8 km s^-1.