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84855502585
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A detailed description of the methods is available in the supplementary materials on
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A detailed description of the methods is available in the supplementary materials on Science Online.
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Science Online
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19
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84878095487
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note
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The distance to the black hole and its line-of-sight velocity cannot be determined, because a measurement of the star's radial velocity is needed for this. S0-102 is currently just beyond the spectroscopic limit.
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20
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84855502585
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S0-104 is a previously unknown detected star; its orbital motion is presented in the supplementary materials on
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S0-104 is a previously unknown detected star; its orbital motion is presented in the supplementary materials on Science Online.
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Science Online
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22
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84878060789
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note
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The strength of the gravitational field we quote here relates to the interbody potential and therefore orbital velocities. However, we want to note that the strong-field internal gravity of the neutron stars could leave imprints on the orbital motion.
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