Evaluating the N/O Chemical Network: The Distribution of N2O and NO in the Sagittarius B2 Complex

Mapping observations of the J = 6 → 5 transition of N 2 O and the Π , J = 3/2 → 1/2 line of NO in the 2 mm band toward the core region of the Sagittarius B2 complex have been carried out using the Kitt Peak 12 m telescope. Emission from NO was found to be extended over a region 2' × 5' in size that includes the Sgr B2 (N), Sgr B2 (M), and Sgr B2 (OH) positions, very similar to the distribution found for HNO. In contrast, N 2 O emission was confined to a source approximately 1' in extent, slightly elongated in the north-south direction and centered on the Sgr B2 (N) core. A virtually identical distribution was found for the J Kτ = 14 0 → 14 -1 E transition of methanol, which lies 255 K above ground state and samples very hot gas. Excitation conditions are favorable for the J = 6 → 5 line of N 2 O over the entire NO region; hence, the confined nature of this species is a result of chemistry. The J = 3 → 2 and J = 9 → 8 lines of N 2 O at 75 and 226 GHz, respectively, were also detected at Sgr B2 (N). Combined with the J = 6 → 5 data, these transitions indicate a column density for this molecule of N tot ~ 1.5 × 10 15 cm -2 at this position and an abundance of f (N 2 O/H 2 ) ~ 1.5 × 10 -9 . This fractional abundance is almost 2 orders of magnitude higher than predicted by low-temperature chemical models. The N 2 O observations suggest that this molecule is preferentially formed in high-temperature gas; a likely mechanism is the neutral-neutral reaction NO + NH → N 2 O + H, which has an appreciable rate only at T > 125 K. The column density of NO found over the Sgr B2 cloud was N tot ~ (0.8-1.5) × 10 16 cm -2 , corresponding to a fractional abundance of f (NO/H 2 ) ~ (0.8-1.5) × 10 -8 , which is about 1 order of magnitude less than model predictions. The similar distributions of NO and HNO suggest a chemical connection. It is likely that the major route to HNO is from NO via the ion-molecule process NO + HNO + → NO + + HNO, which occurs readily at low temperatures. The NO molecule thus appears to be the main precursor species in the N/O chemical network.