Molecular hydrogen emission from protoplanetary disks

被引:118
|
作者
Nomura, H [1 ]
Millar, TJ [1 ]
机构
[1] Univ Manchester, Sch Phys & Astron, Manchester M60 1QD, Lancs, England
关键词
line : formation; molecular processes; radiative transfer; planetary systems : protoplanetary disks;
D O I
10.1051/0004-6361:20052809
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have modeled self-consistently the density and temperature profiles of gas and dust in protoplanetary disks, taking into account irradiation from a central star. Making use of this physical structure, we have calculated the level populations of molecular hydrogen and the line emission from the disks. As a result, we can reproduce the observed strong line spectra of molecular hydrogen from protoplanetary disks, both in the ultraviolet (UV) and the near-infrared, but only if the central star has a strong UV excess radiation.
引用
收藏
页码:923 / U97
页数:20
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