MNRAS 334:646Kusenko A (2009) Sterile neutrinos: the dark side of the light fermions. Here, we will review the complex but well-ordered scenario of the properties of the dark halos also in relation with those of the baryonic components they host. Springer, BerlinMcGaugh SS (2005) The baryonic Tully–Fisher relation of galaxies with extended rotation curves and the stellar mass of rotating galaxies. B) flattened in a disk and about the same size as the stellar disk. ApJ 563:694Viel M, Branchini E, Cen R et al (2005) Tracing the warm-hot intergalactic medium in the local Universe. Two-component mass models, consisting of an exponential disk and a spherical halo, are constructed to fit a newly determined rotation curve of NGC 3198 that extends to 11 disk scale lengths. The distribution of the dark matter in a spiral galaxy is? ApJ 710:903Müller O, Pawlowski MS, Jerjen T et al (2018) A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology. ApJS 99:501Persic M, Salucci P, Stel F (1996) The universal rotation curve of spiral galaxies—I. Contours are -4s, -2s, 2s, 4s, then 10, 15, 20, 30, 50 mJy beamThe rotation curves derived from other methods provided data cubes that were clearly different from those observed. Error budget. A&A 192:117van der Kruit PC, Freeman KC (2011) Galaxy disks. Therefore, for galaxies having Note, however, that this is not entirely true for NGC 1090, in which for some radii the Ha lie ∼10 km sOxford University Press is a department of the University of Oxford.
Cambridge University Press, CambridgeBertone G, Hooper D (2018) History of dark matter. a) approximately spherical and about the same size as the galaxy halo. ... mapping the distribution of globular clusters in the galaxy. ApJ 160:811Freese K (2017) Status of dark matter in the universe. MNRAS 311:441Corsini EM, Wegner GA, Thomas J et al (2017) The density of dark matter haloes of early-type galaxies in low-density environments.
when the velocity field was sufficiently sampled (the case of NGC 1090), we called our method MET (Modified Envelope-Tracing method).
MNRAS 281:27Collaboration Planck, Ade PAR, Aghanim N (2016) Planck 2015 results. Rep Prog Phys 81:066201Rubin VC, Ford WK Jr, Thonnard N (1980) Rotational properties of 21 Sc galaxies with a large range of luminosities and radii, from NGC 4605 (Salucci P (2001) The constant-density region of the dark haloes of spiral galaxies. I. Ultra-diffuse galaxies. MNRAS 474:5259Destri C, de Vega P, Sanchez NG (2013) Warm dark matter primordial spectra and the onset of structure formation at redshift z. PRD 88:3512de Swart J, Bertone G, van Dongen J (2017) How dark matter came to matter.
Since observations of galaxy rotation do not match the distribution expected from application of Kepler's laws, they do not match the distribution of luminous matter.A popular interpretation of these observations is that about 26% of the mass of the Universe is composed of dark matter, a Many cosmologists strive to understand the nature and the history of these ubiquitous dark haloes by investigating the properties of the galaxies they contain (i.e. V. HI rotation curve shapes and the Tully–Fisher relations. AJ 136:2761Oh S-H, Brook C, Governato F (2011) Dark and luminous matter in THINGS dwarf galaxies. JCAP 08(2010):004Catena R, Ullio P (2012) The local dark matter phase-space density and impact on WIMP direct detection. D) flattened in a disk but about ten times larger than the stellar disk. MNRAS 454:1161I thank Francesca Matteucci for motivating me towards the enterprise of writing this review.
The distribution of the non-luminous matter in galaxies of different luminosity and Hubble type is much more than a proof of the existence of dark particles governing the structures of the Universe. According to modern models of physical cosmology, a dark matter halo is a basic unit of cosmological structure. EPJ Web Conf 121:06003García-Bellido J (2017) Massive primordial black holes as dark matter and their detection with gravitational waves. MNRAS 283:837Serra P, Oosterloo T, Cappellari M, den Heijer M, Jozsa GIG (2016) Linear relation between HI circular velocity and stellar velocity dispersion in early-type galaxies, and slope of the density profiles. ARAA 53:51Spano M, Marcelin M, Amram P et al (2008) GHASP: an HSpekkens K, Giovanelli R, Haynes MP (2005) The cusp/core problem in galactic halos: long-slit spectra for a large dwarf galaxy sample.
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