Observations of outflows and disks in pre-main sequence systems

被引：0
|
作者：
Bally, J [1 ]
机构：
[1] Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA
来源：
ACCRETION PROCESSES IN ASTROPHYSICAL SYSTEMS: SOME LIKE IT HOT! | 1998年 / 431期
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The high angular resolution of Hubble Space Telescope has provided stunning evidence for accretion disks around low mass stars and revealed the detailed structure of stellar jets. Large format CCD detectors have been used to show that outflows from young stars can extend parsecs from their sources.
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页码：523 / 532
页数：10
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