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bn:01061629n
Noun Named Entity
Categories: O-type supergiants, Hipparcos objects, Neutron stars, Runaway stars, Objects named with variable star designations
EN
4U 1700-37  4U1700-37  HD 153919  HD 153919/4U 1700-37  V884 Scorpii
EN
4U 1700-37 is one of the stronger binary X-ray sources in the sky, and is classified as a high-mass X-ray binary. Wikipedia
Definitions
Relations
Sources
EN
4U 1700-37 is one of the stronger binary X-ray sources in the sky, and is classified as a high-mass X-ray binary. Wikipedia
IS A
neutron star
H II region
Astrophysical X-ray source
blue supergiant
rotating ellipsoidal variable
+2 relations
EPOCH
J2000.0
Wikipedia
EN
4U 1700-37
Wikidata
EN
4U 1700-37
Wikipedia Redirections
EN
4U1700-37, HD 153919, HD 153919/4U 1700-37, V884 Scorpii

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