phenomenon 50.1 Dark companions too massive to be neutron stars

open in the book · parts/05-general-relativity-cosmology/09-exp-black-holes.tex:372 · p. 1363

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phenomenon 50.1: Dark companions too massive to be neutron stars50.1phenomenon 27.35: Kepler's third law27.35theorem 27.30: Reduction of the two-body problem27.30proof : ch:09-exp-black-holes@proof-1proofequation 27.47: eq:cfs-conic27.47equation 27.22: eq:cfs-kepler-second27.22phenomenon 50.5: Black-hole masses from gravitational waves50.5phenomenon 50.2: Four million solar masses inside the orbit of a single star50.2proof : ch:10-central-forces-statics@proof-21proofequation 19.38: eq:newt-cm-position19.38equation 19.4: eq:newt-fma19.4postulate 19.48: Newton's third law19.48phenomenon 27.32: Kepler's first law: bound orbits are closed ellipses27.32proof : ch:10-central-forces-statics@proof-18proof

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cites (evidence) Identification of Cygnus X-1 with HDE 226868 derived parts/05-general-relativity-cosmology/09-exp-black-holes.tex:377
cites (evidence) A 6.5-day periodicity in the recurrent nova V404 Cygni implying the presence of a black hole derived parts/05-general-relativity-cosmology/09-exp-black-holes.tex:385
cites (evidence) Cygnus X-1 contains a 21--solar mass black hole---Implications for massive star winds derived parts/05-general-relativity-cosmology/09-exp-black-holes.tex:379
cites (data) X-Ray Properties of Black-Hole Binaries derived parts/05-general-relativity-cosmology/09-exp-black-holes.tex:385
cites (evidence) Cygnus X-1---a Spectroscopic Binary with a Heavy Companion ? derived parts/05-general-relativity-cosmology/09-exp-black-holes.tex:377
depends_on Kepler's third law declared parts/05-general-relativity-cosmology/09-exp-black-holes.tex:388
depends_on Reduction of the two-body problem declared parts/05-general-relativity-cosmology/09-exp-black-holes.tex:388
proves ch:09-exp-black-holes@proof-1 declared parts/05-general-relativity-cosmology/09-exp-black-holes.tex:391