Direct Evidence;
Radial Velocity;
System Type;
Planetary System;
Surprising Diversity;
D O I:
10.1023/A:1008327904217
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
The past decade brought direct evidence of the previously surmised exoplanetary systems. A variety of planetary system types exist: those around pulsars, around both young and old main-sequence stars (as evidenced by planetesimal disks of the Beta Pictoris-type), and the mature giant exoplanets found in radial velocity surveys. The surprising diversity of the exoplanetary systems is addressed by several theories of their origin.
机构:
Univ Sao Paulo, Inst Astron Geofis & Ciencias Astmosfer, Sao Paulo, BrazilUniv Sao Paulo, Inst Astron Geofis & Ciencias Astmosfer, Sao Paulo, Brazil
Ferraz-Mello, S
Michtchenko, TA
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h-index: 0
机构:
Univ Sao Paulo, Inst Astron Geofis & Ciencias Astmosfer, Sao Paulo, BrazilUniv Sao Paulo, Inst Astron Geofis & Ciencias Astmosfer, Sao Paulo, Brazil
Michtchenko, TA
Beaugé, C
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h-index: 0
机构:
Univ Sao Paulo, Inst Astron Geofis & Ciencias Astmosfer, Sao Paulo, BrazilUniv Sao Paulo, Inst Astron Geofis & Ciencias Astmosfer, Sao Paulo, Brazil
Beaugé, C
Callegari, N
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h-index: 0
机构:
Univ Sao Paulo, Inst Astron Geofis & Ciencias Astmosfer, Sao Paulo, BrazilUniv Sao Paulo, Inst Astron Geofis & Ciencias Astmosfer, Sao Paulo, Brazil
Callegari, N
[J].
CHAOS AND STABILITY IN PLANETARY SYSTEMS,
2005,
683
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271