Description
Metadata
Settings
owl:sameAs
Inference Rule:
b3s
b3sifp
facets
http://www.w3.org/2002/07/owl#
ldp
oplweb
skos-trans
virtrdf-label
None
About:
dbkwik:resource/0eDghR2TBtefSOwEtxtkcg==
Sponge
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An Entity of Type :
owl:Thing
, within Data Space :
134.155.108.49:8890
associated with source
dataset(s)
Attributes
Values
rdfs:label
脉冲星
rdfs:comment
脉冲星,发现于1967年,脉冲星会发出周期性的电波,会发出强烈的电磁脉冲信号。脉冲星自转速度比中子星还要快,因此99%的脉冲星都会呈现椭球体。绝大多数的脉冲星属于中子星。
dcterms:subject
dbkwik:resource/XfoRIDP61v_kp902UflWjg==
dbkwik:resource/xIlaEB27HyhrL_CbZSB3GA==
abstract
脉冲星,发现于1967年,脉冲星会发出周期性的电波,会发出强烈的电磁脉冲信号。脉冲星自转速度比中子星还要快,因此99%的脉冲星都会呈现椭球体。绝大多数的脉冲星属于中子星。
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