The glycolaldehyde is detected towards the Galactic center source Sgr B2(N) and towards the massive star-forming region G31.41+0.31 through b-type transitions. The levels for b-type transitions can be classified into two groups: (i) with ka+kc = odd (set I) and (ii) with ka+kc = even (set II). For each of the sets I and II, we have calculated energies of 100 rotational levels. These levels are connected through radiative and collisional transitions. The Einstein A-coefficients for the radiative transitions among the levels are calculated. The collisional rate coefficients are calculated with the help of a scaling law. Using the radiative and collisional transitions probabilities, for each of the sets I and II, we have solved a set of statistical equilibrium equations coupled with the equations of radiative transfer. Two transitions 110−101 and 312−303 at 13.477 GHz and 17.981 GHz, respectively, of set I, and one transition 211−202 at 15.176 GHz of set II are found to have anomalous absorption. These transitions may play important role in the identification of glycolaldehyde in a cosmic object.
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