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Three micron ice-band features in the Rho Ophiuchi sources
The Astrophysical Journal1990Vol. 352, pp. 724–724
Citations Over TimeTop 10% of 1990 papers
Abstract
Low-resolution spectra in the 2.4-3.8 micron range are presented for 31 sources in the Rho Oph dark cloud. The characteristics of the 3-micron spectra for protostars, emission-line stars, associated early-type stars, and background M giant stars are examined. Consideration is given to the relationship between ice-band absorption and H-K magnitude. The results show the existence of ice-mantled grains in the circumstellar disks of emission-line stars. The processes controling the formation of H2O ice in dark clouds are discussed.
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