共 50 条
X-rays and Protoplanetary Disks
被引:0
|作者:
Skinner, S. L.
[1
]
Guedel, M.
[2
]
Briggs, K. R.
[2
]
Audard, M.
[3
,4
]
Lamzin, S. A.
[5
]
Sokal, K. R.
[1
]
机构:
[1] Univ Colorado, CASA, Boulder, CO 80309 USA
[2] ETH, Inst Astron, Zurich, Switzerland
[3] Univ Geneva, ISDC, Geneva, Switzerland
[4] Univ Geneva, Observ Geneva, Geneva, Switzerland
[5] Sternberg Astron Inst, Moscow, Russia
来源:
关键词:
stars:pre-main-sequence;
x-rays:stars;
YOUNG STELLAR OBJECTS;
EMISSION;
TAURI;
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
X-ray luminosities of T Tauri stars (TTS) and Class I protostars are commonly elevated by a thousand-fold above that of the present-day Sun. They undergo frequent powerful x-ray flares which can reach temperatures of similar to 100 MK, exposing the disk to intense bursts of ionizing radiation and high-energy particles. We provide a brief overview of how x-rays can affect protoplanetary disks and summarize x-ray diagnostics that can be used to infer disk properties. Representative x-ray observations of accreting young stellar objects with XMM-Newton and Chandra are discussed.
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页码:157 / +
页数:2
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