(en) Christoph Perrot et Isabelle Grenier, « 3D dynamical evolution of the interstellar gas in the Gould Belt », Astromy & Astrophysics, vol. 404, (lire en ligne)
(en) John F. W. Herschel, Results of astronomical observations made during the years 1834, 5 ,6, 7, 8, at the Cape of Good Hope, Londres, Smith, Elder & Co., (DOI10.3931/e-rara-22242, Bibcode1847QB3.H52........), no 321, p. 385 (lire en ligne [html]) : « the zone of large stars wich is marked out by the briliant constellation of Orion, the bright stars of Canis Major, and almost more conspicuous stars of Argo–the Cross–the Centaur, Lupus, and Scorpio. A great circle passing through ε Orionis and α Crucis will mark out the axis of the zone in question, whose inclination to the galactic circle is therefore about 20°, and whose appearance would lead us to suspect that our nearest neighbours in the sideral system (if really such), form part of a subordonate sheet or stratum deviating to that extent from parallelism to the general mass which, seen projected on the heavens, form the Milky Way. »
esa.int
rssd.esa.int
(en) « The Gould Belt », The GAIA Study Report (consulté le )
eso.org
Christoph Perrot et Isabelle Grenier, 3D évolution of the Gould Belt, 2001 (en) [2](dossier de l'Observatoire européen austral]) consulté en ligne le 15 janvier 2023
(en) John F. W. Herschel, Results of astronomical observations made during the years 1834, 5 ,6, 7, 8, at the Cape of Good Hope, Londres, Smith, Elder & Co., (DOI10.3931/e-rara-22242, Bibcode1847QB3.H52........), no 321, p. 385 (lire en ligne [html]) : « the zone of large stars wich is marked out by the briliant constellation of Orion, the bright stars of Canis Major, and almost more conspicuous stars of Argo–the Cross–the Centaur, Lupus, and Scorpio. A great circle passing through ε Orionis and α Crucis will mark out the axis of the zone in question, whose inclination to the galactic circle is therefore about 20°, and whose appearance would lead us to suspect that our nearest neighbours in the sideral system (if really such), form part of a subordonate sheet or stratum deviating to that extent from parallelism to the general mass which, seen projected on the heavens, form the Milky Way. »
(en) John F. W. Herschel, Results of astronomical observations made during the years 1834, 5 ,6, 7, 8, at the Cape of Good Hope, Londres, Smith, Elder & Co., (DOI10.3931/e-rara-22242, Bibcode1847QB3.H52........), no 321, p. 385 (lire en ligne [html]) : « the zone of large stars wich is marked out by the briliant constellation of Orion, the bright stars of Canis Major, and almost more conspicuous stars of Argo–the Cross–the Centaur, Lupus, and Scorpio. A great circle passing through ε Orionis and α Crucis will mark out the axis of the zone in question, whose inclination to the galactic circle is therefore about 20°, and whose appearance would lead us to suspect that our nearest neighbours in the sideral system (if really such), form part of a subordonate sheet or stratum deviating to that extent from parallelism to the general mass which, seen projected on the heavens, form the Milky Way. »
articles.adsabs.harvard.edu
Carlos Alberto Olano, « On a Model of Local Gas Related to Gould's Belt », Astronomy & Astrophysics, vol. 112, , p. 195 - 208 (lire en ligne)
harvardmagazine.com
(en) Bennett McIntosh, « An Interstellar Ribbon of Clouds in the Sun's Backyard », Harvard Magazine, (lire en ligne)
Agence spatiale européenne, 3-D visualisation redefines Milky Way's local architecture, dans la revue Phys.Org, le 16 novembre 2015 (en) [3]
physicsworld.com
Physics World, Superbubble region of star formation was created by supernovae, study suggests, le 11 octobre 2021 (en) [4]
sites.google.com
La ceinture de Gould que Perrot et Grenier ont localisée, est présentée en 3D, dans l'optique de comparaison, par le site de l'université Harvard : voir la première image en 3D (Explore the RadWave in 3D), puis rubrique Gould's Belt (Perrot & Grenier 2003)[1]
