Abstract
Various complex molecules were only detected toward the Sgr B2(N) dense core. Together with other observational evidence for the existence of warm core-mantle grains in Sgr B2(N), we believe this is due to abundance variations as a result of enhanced grain-surface chemistry.
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© 1996 Springer-Verlag Berlin Heidelberg
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Kuan, YJ., Snyder, L.E., Miao, Y., Mehringer, D.M. (1996). Interferometric Observations of Sagittarius B2: Evidence for Grain Chemistry. In: Shaver, P.A. (eds) Science with Large Millimetre Arrays. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-69999-6_29
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DOI: https://doi.org/10.1007/978-3-540-69999-6_29
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