Evidence for grain growth in the protostellar disks of Orion

被引:32
|
作者
Shuping, RY [1 ]
Bally, J
Morris, M
Throop, H
机构
[1] Univ Calif Los Angeles, Div Astron & Astrophys, Los Angeles, CA 90095 USA
[2] Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA
[3] SW Res Inst, Dept Space Studies, Boulder, CO 80302 USA
来源
ASTROPHYSICAL JOURNAL | 2003年 / 587卷 / 02期
关键词
circumstellar matter; dust; extinction; stars : formation; stars : pre-main-sequence;
D O I
10.1086/375334
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a Bralpha (lambda = 4.05 mum) image of the largest silhouette proplyd in Orion (114-426) using the facility near-IR spectrometer NIRSPEC at the Keck Observatory. This is the longest wavelength observation of a silhouette disk to date. The diameter of the disk at 4 mum is only marginally smaller than that observed in the optical with the Hubble Space Telescope. This may be the first signature of chromatic extinction for the translucent outer edges of the disk, suggesting that the near- IR opacity is dominated by processed grains with typical sizes greater than 1.9 mum, but not >>4 mum.
引用
收藏
页码:L109 / L112
页数:4
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