Lenticular vs spiral galaxies: dark matter content and the Tully-Fisher relation

Lenticular vs spiral galaxies: dark matter content and the Tully-Fisher relation

Bibliográfalaš dieđut
Váldodahkkit:	Bureau, M, Williams, M, Cappellari, M
Materiálatiipa:	Conference item
Almmustuhtton:	2010

Geahča maid

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Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies
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HI Linewidths, Rotation Velocities and the Tully-Fisher Relation
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The MBHBM* project - II. Molecular gas kinematics in the lenticular galaxy NGC 3593 reveal a supermassive black hole
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The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully-Fisher relation at z ~ 1
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The Baryonic Tully–Fisher Relation. II. Stellar Mass Models
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Modified Newtonian Gravity, Wide Binaries and the Tully-Fisher Relation
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A Generalist, Automated ALFALFA Baryonic Tully–Fisher Relation
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The multiwavelength Tully–Fisher relation with spatially resolved H i kinematics
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Six spiral galaxies lacking dark matter
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Analysis of dark matter profiles in the halos of spiral galaxies
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The Tully–Fisher and mass–size relations from halo abundance matching
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The scatter, residual correlations and curvature of the sparc baryonic Tully–Fisher relation
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The SAURON project - VI. Line strength maps of 48 elliptical and lenticular galaxies
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Hints for a Gravitational Transition in Tully–Fisher Data
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THE ASSEMBLY HISTORY OF DISK GALAXIES. I. THE TULLY-FISHER RELATION TO z similar or equal to 1.3 FROM DEEP EXPOSURES WITH DEIMOS
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Neutral hydrogen in nearby elliptical and lenticular galaxies: the continuing formation of early-type galaxies
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The new semi-analytic code GalICS 2.0 – reproducing the galaxy stellar mass function and the Tully–Fisher relation simultaneously
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