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- 4U_1700-37 abstract "4U 1700-37 is one of the stronger binary X-ray sources in the sky. It was discovered by the Uhuru satellite. The "4U" designation refers to the Fourth (and final) Uhuru catalog.It is associated with a bright (6.53 V magnitude) supergiant Of star HD 153919, which is orbited by an accreting compact object that must be either a neutron star or a black hole.The X-ray source is eclipsed by the star every ~3.4 days, but no pulsations have yet been observed.The source is one of the ten brightest persistent X-ray sources in the 10-100 keV hard X-ray energy region.".
- 4U_1700-37 wikiPageID "18213622".
- 4U_1700-37 wikiPageRevisionID "568843060".
- 4U_1700-37 hasPhotoCollection 4U_1700-37.
- 4U_1700-37 subject Category:Binary_stars.
- 4U_1700-37 subject Category:Henry_Draper_Catalogue_objects.
- 4U_1700-37 subject Category:Neutron_stars.
- 4U_1700-37 subject Category:Objects_named_with_variable_star_designations.
- 4U_1700-37 comment "4U 1700-37 is one of the stronger binary X-ray sources in the sky. It was discovered by the Uhuru satellite.".
- 4U_1700-37 label "4U 1700-37".
- 4U_1700-37 sameAs m.04ct606.
- 4U_1700-37 sameAs Q4638996.
- 4U_1700-37 sameAs Q4638996.
- 4U_1700-37 wasDerivedFrom 4U_1700-37?oldid=568843060.
- 4U_1700-37 isPrimaryTopicOf 4U_1700-37.