Discovery of Crystallized Water Ice in a Silhouette Disk in the M43 Region
Hiroshi Terada, Alan T. Tokunaga

TL;DR
This study reports the first direct detection of crystallized water ice in a silhouette disk, revealing how disk inclination affects water ice absorption and indicating grain growth on the disk surface.
Contribution
It provides new evidence of crystallized water ice in a silhouette disk and identifies the critical inclination angle for water ice absorption strength.
Findings
Water ice absorption detected in two of five stars.
Disk inclination angle influences water ice optical depth.
Crystallized water ice with grain growth observed on disk surface.
Abstract
We present the 1.9--4.2um spectra of the five bright (L<11.2) young stars associated with silhouette disks with moderate to high inclination angle of 39--80deg in the M42 and M43 regions. The water ice absorption is seen toward d121-1925 and d216-0939, while the spectra of d182-316, d183-405, and d218-354 show no water ice feature around 3.1um within the detection limits. By comparing the water ice features toward nearby stars, we find that the water ice absorption toward d121-1925 and d216-0939 most likely originates from the foreground material and the surrounding disk, respectively. The angle of the disk inclination is found to be mainly responsible for the difference of the optical depth of the water ice among the five young stars. Our results suggest that there is a critical inclination angle between 65deg and 75deg for the circumstellar disk where the water ice absorption becomes…
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