Garrett, Katherine; Dūda, Gintaras. Dark Matter: A
Primer // Advances in Astronomy. — Т. 2011. — С. 968283. — doi:10.1155/2011/968283. — Bibcode: 2011AdAst2011E...8G. — arXiv:1006.2483.. p. 3: "MACHOs can only account for a very small percentage of the nonluminous mass in our galaxy, revealing that most dark matter cannot be strongly concentrated or exist in the form of baryonic astrophysical objects. Although microlensing surveys rule out baryonic objects like brown dwarfs, black holes, and neutron stars in our galactic halo, can other forms of baryonic matter make up the bulk of dark matter? The answer, surprisingly, is no..."
Blumenthal, George R.; Pagels, Heinz; Primack, Joel R. Galaxy formation by dissipationless particles heavier than
neutrinos (англ.) // Nature : journal. — 1982. — 2 September (vol. 299, no. 5878). — P. 37—38. — doi:10.1038/299037a0. — Bibcode: 1982Natur.299...37B.
Blumenthal, G. R.; Faber, S. M.; Primack, J. R.; Rees,, M. J. Formation of galaxies and large-scale structure with
cold dark matter (англ.) // Nature : journal. — 1984. — Vol. 311, no. 517. — P. 517—525. — doi:10.1038/311517a0. — Bibcode: 1984Natur.311..517B.
Garrett, Katherine; Dūda, Gintaras. Dark Matter: A
Primer // Advances in Astronomy. — Т. 2011. — С. 968283. — doi:10.1155/2011/968283. — Bibcode: 2011AdAst2011E...8G. — arXiv:1006.2483.. p. 3: "MACHOs can only account for a very small percentage of the nonluminous mass in our galaxy, revealing that most dark matter cannot be strongly concentrated or exist in the form of baryonic astrophysical objects. Although microlensing surveys rule out baryonic objects like brown dwarfs, black holes, and neutron stars in our galactic halo, can other forms of baryonic matter make up the bulk of dark matter? The answer, surprisingly, is no..."
Blumenthal, George R.; Pagels, Heinz; Primack, Joel R. Galaxy formation by dissipationless particles heavier than
neutrinos (англ.) // Nature : journal. — 1982. — 2 September (vol. 299, no. 5878). — P. 37—38. — doi:10.1038/299037a0. — Bibcode: 1982Natur.299...37B.
Blumenthal, G. R.; Faber, S. M.; Primack, J. R.; Rees,, M. J. Formation of galaxies and large-scale structure with
cold dark matter (англ.) // Nature : journal. — 1984. — Vol. 311, no. 517. — P. 517—525. — doi:10.1038/311517a0. — Bibcode: 1984Natur.311..517B.
Garrett, Katherine; Dūda, Gintaras. Dark Matter: A
Primer // Advances in Astronomy. — Т. 2011. — С. 968283. — doi:10.1155/2011/968283. — Bibcode: 2011AdAst2011E...8G. — arXiv:1006.2483.. p. 3: "MACHOs can only account for a very small percentage of the nonluminous mass in our galaxy, revealing that most dark matter cannot be strongly concentrated or exist in the form of baryonic astrophysical objects. Although microlensing surveys rule out baryonic objects like brown dwarfs, black holes, and neutron stars in our galactic halo, can other forms of baryonic matter make up the bulk of dark matter? The answer, surprisingly, is no..."
