The Baryonic Tully-Fisher Relation of Gas Rich Galaxies as a Test of LCDM and MOND

Abstract

The Baryonic Tully-Fisher Relation (BTFR) is an empirical relation between baryonic mass and rotation velocity in disk galaxies. It provides tests of galaxy formation models in LCDM and of alternative theories like MOND. Observations of gas rich galaxies provide a measure of the slope and normalization of the BTFR that is more accurate (if less precise) than that provided by star dominated spirals, as their masses are insensitive to the details of stellar population modeling. Recent independent data for such galaxies are consistent with Mb = AVf^4 with A = 47+/-6 Msun (km/s)^-4. This is equivalent to MOND with $a_0 = 1.3 +/- 0.3 A/s/s. The scatter in the data is consistent with being due entirely to observational uncertainties. It is unclear why the physics of galaxy formation in LCDM happens to pick out the relation predicted by MOND. We introduce a feedback efficacy parameter E to relate halo properties to those of the galaxies they host. E correlates with star formation rate and gas fraction in the sense that galaxies that have experienced the least star formation have been most impacted by feedback.

Astronomical Journal, in press. Added new figure (7 total); new version matches accepted version. Electronic data available at http://www.astro.umd.edu/~ssm/data/gasrichdatatable.txt

References in corpus (27)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
• High-Resolution Rotation Curves and Galaxy Mass Models from THINGS
• Dark Matter Results from 100 Live Days of XENON100 Data
• Forming Disk Galaxies in Lambda CDM Simulations
• High-resolution dark matter density profiles of THINGS dwarf galaxies: Correcting for non-circular motions
• Scaling Relations of Spiral Galaxies
• FIGGS: Faint Irregular Galaxies GMRT Survey - Overview, observations and first results
• NGC 3741: dark halo profile from the most extended rotation curve
• The rotation curves shapes of late-type dwarf galaxies
• Do Hot Haloes Around Galaxies Contain the Missing Baryons?
• A Novel Test of the Modified Newtonian Dynamics with Gas Rich Galaxies
• Fitting galactic rotation curves with conformal gravity and a global quadratic potential
• Optical-to-virial velocity ratios of local disk galaxies from combined kinematics and galaxy-galaxy lensing
• A First Attempt to Calibrate the Baryonic Tully-Fisher Relation with Gas Dominated Galaxies
• THINGS about MOND
• A Survey of Galaxy Kinematics to z ~ 1 in the TKRS/GOODS-N Field. II. Evolution in the Tully-Fisher Relation
• Where are the Fossils of the First Galaxies? II. True Fossils, Ghost Halos, and the Missing Bright Satellites
• The emptiness of voids: yet another over-abundance problem for the LCDM model
• Baryonic Tully-Fisher Relation for Extremely Low Mass Galaxies
• Do Baryons Alter the Halos of Low Surface Brightness Galaxies?
• The high mass end of the Tully-Fisher relation
• Dark Matter Halos of Disk Galaxies: Constraints from the Tully-Fisher Relation
• GHASP: an Hα kinematic survey of spiral and irregular galaxies -- IX. The NIR, stellar and baryonic Tully-Fisher relations
• The Radial Tully-Fisher relation for spiral galaxies I
• CO Detection and Millimeter Continuum Emission from Low Surface Brightness Galaxies
• Testing Modified Gravity (MOG) with gas-dominated galaxies

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• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
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• Towards a more realistic population of bright spiral galaxies in cosmological simulations
• Third-Epoch Magellanic Cloud Proper Motions II: The Large Magellanic Cloud Rotation Field in Three Dimensions
• Small scale problems of the $\Lambda$CDM model: a short review
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• Star-Forming Galaxies at Cosmic Noon
• The dark matter crisis: falsification of the current standard model of cosmology
• Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time
• Dark matter, dark energy, and alternate models: A review
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