Analysis of information sources in references of the Wikipedia article "Cold dark matter" in English language version.
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: CS1 maint: article number as page number (link)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' ...
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: CS1 maint: article number as page number (link){{cite journal}}
: CS1 maint: article number as page number (link)Dwarf galaxies play a crucial role in the CDM scenario for galaxy formation, having been suggested to be the natural building blocks from which larger structures are built up by merging processes. In this scenario dwarf galaxies are formed from small-scale density fluctuations in the primeval universe.
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: CS1 maint: bot: original URL status unknown (link){{cite journal}}
: CS1 maint: article number as page number (link)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' ...
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: CS1 maint: article number as page number (link){{cite journal}}
: CS1 maint: article number as page number (link)Dwarf galaxies play a crucial role in the CDM scenario for galaxy formation, having been suggested to be the natural building blocks from which larger structures are built up by merging processes. In this scenario dwarf galaxies are formed from small-scale density fluctuations in the primeval universe.
{{cite journal}}
: CS1 maint: bot: original URL status unknown (link){{cite journal}}
: CS1 maint: article number as page number (link)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' ...
{{cite journal}}
: CS1 maint: article number as page number (link){{cite journal}}
: CS1 maint: article number as page number (link){{cite journal}}
: CS1 maint: article number as page number (link){{cite journal}}
: CS1 maint: article number as page number (link)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' ...
{{cite journal}}
: CS1 maint: article number as page number (link){{cite journal}}
: CS1 maint: article number as page number (link)Dwarf galaxies play a crucial role in the CDM scenario for galaxy formation, having been suggested to be the natural building blocks from which larger structures are built up by merging processes. In this scenario dwarf galaxies are formed from small-scale density fluctuations in the primeval universe.
{{cite journal}}
: CS1 maint: bot: original URL status unknown (link)