Results 291 to 300 of about 527,839 (302)
A temperate super-Jupiter imaged with JWST in the mid-infrared. [PDF]
Matthews EC+18 more
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Identification of a turnover in the initial mass function of a young stellar cluster down to 0.5 MJ
De Furio M+13 more
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Compact stars with non-uniform relativistic polytrope. [PDF]
Nouh MI, Foda MM, Aboueisha MS.
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On networks of space-based gravitational-wave detectors. [PDF]
Cai RG+9 more
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Baryonic solutions and challenges for cosmological models of dwarf galaxies
Nature Astronomy, 2022Galaxies and their dark-matter haloes have posed several challenges to the dark energy plus cold dark matter (ΛCDM) cosmological model. These discrepancies between observations and theory intensify for the lowest-mass (‘dwarf’) galaxies. ΛCDM predictions
L. Sales, A. Wetzel, Azadeh Fattahi
semanticscholar +1 more source
Hunting for massive black holes in dwarf galaxies
Nature Astronomy, 2022Despite traditional thinking, an appreciable population of massive black holes (that is, more massive than stellar-mass black holes) may be lurking in dwarf galaxies.
A. Reines
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Further evidence for a population of dark-matter-deficient dwarf galaxies
Nature Astronomy, 2019In the standard cosmological model, dark matter drives the structure formation of galaxies and constructs potential wells within which galaxies may form.
Q. Guo+11 more
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2004
Dwarf irregular galaxies at optical wavelengths are small, faint and appear to be unstructured and irregular in shape. They are typically gas-rich, metal-poor systems, with varying levels of STAR FORMATION occurring in a haphazard manner across the ...
openaire +3 more sources
Dwarf irregular galaxies at optical wavelengths are small, faint and appear to be unstructured and irregular in shape. They are typically gas-rich, metal-poor systems, with varying levels of STAR FORMATION occurring in a haphazard manner across the ...
openaire +3 more sources
Suppression of star formation in dwarf galaxies by photoelectric grain heating feedback
Nature, 2016Photoelectric heating—heating of dust grains by far-ultraviolet photons—has long been recognized as the primary source of heating for the neutral interstellar medium.
John C. Forbes+3 more
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