ALMA and the Future of Millimeter Imaging Observations

被引:0
|
作者
Wilner, David J. [1 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
来源
YOUNG STARS & PLANETS NEAR THE SUN | 2016年 / 10卷 / 314期
关键词
circumstellar matter; planet-disk interactions; submillimeter: planetary systems;
D O I
10.1017/S1743921315006080
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Nearby Young Moving Groups sample the critical age when primordial disks around stars complete their transformation into planetary systems with associated debris. Millimeter wavelengths provide direct access to cool material in these circumstellar disks. The high angular resolution of interferometry at these long wavelengths enables resolved observations of solids in an optically thin regime, as well as the thermal, chemical, and dynamical structure of gas, if present. In this contribution, I briefly review the evolving landscape of millimeter telescopes, with emphasis on the revolutionary capabilities of the new international Atacama Large Millimeter/submillimeter Array (ALMA) and describe pertinent early science results.
引用
收藏
页码:270 / 275
页数:6
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