Thermal radiation from isolated neutron stars

被引：0
|
作者：
Zavlin, VE [1 ]
机构：
[1] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA
[2] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
来源：
HIGHLY ENERGETIC PHYSICAL PROCESSES AND MECHANISMS FOR EMISSION FROM ASTROPHYSICAL PLASMAS | 2000年 / 195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 analysis of thermal radiation emitted from the atmospheres of isolated neutron stars allows one to measure their surface temperatures, magnetic fields, masses, and radii, as well as the chemical composition of their atmospheres. Thus, multiwavelength observations of this radiation provide an important tool for studying the structure and evolution of neutron stars and for elucidating properties of the superdense matter in their interiors. We describe recent theoretical and observational results on thermal radiation from radio pulsars and radio-quiet neutron stars and discuss their astrophysical implications.
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页码：103 / 112
页数：10
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