The H2S 22,0 - 21,1 line emission is observed to be strongly localized toward Sgr B2(M), and emissions from other positions in the more extended SgrB2 region are almost negligible. H2S is thought to form effectively by the passage of the C-type shocks but to be quickly transformed to SO2 or other sulfur species (Pineau des Forets et al. 1993). Such a shock may have enhanced the H2S abundance in Sgr B2(M), where massive star formation is taking place. But the negligible emission of H2S from other observed positions may indicate that these positions have not been affected by shocks enough to produce H2S, or if they have experienced shocks, H2S may have transformed already to other sulfur-containing species. The SO2 222,20 - 221,21 line was also observed to be detectable only toward the (M) position. The line intensity ratios of these two molecules appear to be very similar at Sgr B2(M) and IRAS 16239-2422, where the latter is a region of low-mass star formation. This may suggest that the shock environment in these two star-forming regions is similar and that the shock chemistry also proceeds in a similar fashion in these two different regions, if we accept shock formation of these two species.

비다공성막을 통한 기체 투광성분의 투과 transient와 투과 조성을 on-line 방식으로 측정할 수 있는 기체 투과장치를 개발하였다. 측정은 연속흐름방식으로 이루어지며 측정한 투과 transien로부터 여러 가지의 투과특성, 즉, 투과계수, 확산계수, 용해계수 등을 동시에 평가할 수 있다. 잘 알려진 유리상 고분자인 두 가지 폴리이드막과 고무상의 고분자인 실리콘막을 선택하여 여러 가지의 기체투과 특성들을 측정하여 문헌치와 비교함으로써 투과장치 및 측정방법에 대한 신뢰성, 정확성을 확인하였다. 또한 측정한 투과 transient를 분석함으로써 막을 통한 기체 투과거동을 좀더 자세하게 다양하게 분석할 수가 있다.