NAOC Open IR
晚型巨星FK Com的射电观测研究
Mutel R L1; 皇甫文忠2; 李永生2; 苏步美2
1995
Source Publication天文学报
ISSN0001-5245
Volume036Issue:001Pages:30
Abstract本文作者使用美国VLA,对快速自转的晚型巨星FKCom在3.6、6、18、20cm波长上进行了射电观测,探讨到mjy量级的射电辐射,而没有探测到圆偏振。我们用热模型对射电频谱进行了拟合,结果都不成功。当发射体内电子密度为9×10^8cm^-3,温度为5×10^7K时,半径为120R。可获得较为接近的流量,但10^9量级的电子密度不大可能扩展到如此大的范围,这样的发射体用热模型得到的X射线光度比Ei
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/41305
Collection中国科学院国家天文台
Affiliation1.美国依阿华大学
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
Mutel R L,皇甫文忠,李永生,等. 晚型巨星FK Com的射电观测研究[J]. 天文学报,1995,036(001):30.
APA Mutel R L,皇甫文忠,李永生,&苏步美.(1995).晚型巨星FK Com的射电观测研究.天文学报,036(001),30.
MLA Mutel R L,et al."晚型巨星FK Com的射电观测研究".天文学报 036.001(1995):30.
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