IDENTIFICATION OF THE GUEST STAR OF AD-185 AS A COMET RATHER THAN A SUPERNOVA

被引:27
作者
CHIN, YN [1 ]
HUANG, YL [1 ]
机构
[1] NATL TSING HUA UNIV,HIST INST,HSINCHU 30043,TAIWAN
关键词
D O I
10.1038/371398a0
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
VERY few nearby supernovae have been bright enough to see with the naked eye. The only such case this century was supernova 1987A. Matching historical records of such events with presently observable remnants allows accurate estimates to be made of the age and incidence rate of supernovae; ancient Chinese astronomical records are a particularly valuable resource for this purpose. The Houhanshu(1) of the Later Han dynasty records the appearance of a 'guest star' in AD 185. This is widely regarded as the oldest supernova recorded historically, and several candidate remnants have been suggested(2,3), in particular the object RCW86(2). Here we show that a reinterpretation of the relevant passage in the Houhanshu is inconsistent with the supernova interpretation, but suggests instead that the guest star was a comet. Our findings indicate that some of the keywords used by Chinese astronomers in historical records must be interpreted with caution.
引用
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页码:398 / 399
页数:2
相关论文
共 23 条
[1]  
CHEN ML, QIANXIANGDIAN GUJIN, V10, P53
[2]  
Clark D., 1977, HIST SUPERNOVAE
[3]  
Duyvenday J. J.L., 1942, PASP, V54, P91
[4]  
FAN Y, HOUHANSHU, V6, P3230
[5]  
FAN Y, 1971, HOUHANSHU, V6, P3260
[6]  
FAN Y, HOUHANSHU, V6, P3256
[7]  
Ho P. Y., 1962, VISTAS ASTRON, V5, P127, DOI [10.1016/0083-6656(62)90007-7, DOI 10.1016/0083-6656(62)90007-7]
[8]   A REVISIT TO THE GUEST STAR OF AD185 [J].
HUANG, YL ;
MORIARTYSCHIEVEN, GH .
SCIENCE, 1987, 235 (4784) :59-60
[9]  
KAASTRA JS, 1992, ASTRON ASTROPHYS, V264, P654
[10]  
Lundmark K., 1921, PUBL ASTRON SOC PAC, V33, P225, DOI [10.1086/123101, DOI 10.1086/123101]