(en) R. Abuter et al. (collaboration GRAVITY), « Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole », Astronomy and Astrophysics, vol. 615, , p. 1-10, article no L15 (DOI10.1051/0004-6361/201833718, lire en ligne [PDF]).
(en) collaboration GRAVITY, « Detection of the Schwarzschild precession in the orbit of the star S2 near the Galactic centre massive black hole », Astronomy and Astrophysics, vol. 636, (lire en ligne), accès libre.
Becerra-Vergara et al., Geodesic motion of S2 and G2 as test of the fermionic dark matter nature of our Galactic core, dans le site Astronomy & Astrophsics, le 4 septembre 2020 (en) [2] ; voir aussi l'article scientifique par Ryan Whitwam, The Milky Way Might Have a Core of Dark Matter instead of a Black Hole, le 24 mai 2021 (en) [3]
(en) R. Abuter et al. (collaboration GRAVITY), « Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole », Astronomy and Astrophysics, vol. 615, , p. 1-10, article no L15 (DOI10.1051/0004-6361/201833718, lire en ligne [PDF]).
Becerra-Vergara et al., Geodesic motion of S2 and G2 as test of the fermionic dark matter nature of our Galactic core, dans le site Astronomy & Astrophsics, le 4 septembre 2020 (en) [2] ; voir aussi l'article scientifique par Ryan Whitwam, The Milky Way Might Have a Core of Dark Matter instead of a Black Hole, le 24 mai 2021 (en) [3]
nobelprize.org
Académie royale des sciences de Suède, The Nobel Prize in Physics 2020, le 6 octobre 2020 : « The orbits of the brightest stars closest to the middle of the Milky Way have been mapped with increasing precision. » (en) [5]
