SIMBAD references

2012MNRAS.425.2299S - Mon. Not. R. Astron. Soc., 425, 2299-2308 (2012/September-3)

The link between the baryonic mass distribution and the rotation curve shape.

SWATERS R.A., SANCISI R., VAN DER HULST J.M. and VAN ALBADA T.S.

Abstract (from CDS):

The observed rotation curves of disc galaxies, ranging from late-type dwarf galaxies to early-type spirals, can be fitted remarkably well simply by scaling up the contributions of the stellar and HI discs. This `baryonic scaling model' can explain the full breadth of observed rotation curves with only two free parameters. For a small fraction of galaxies, in particular early-type spiral galaxies, HI scaling appears to fail in the outer parts, possibly due to observational effects or ionization of HI. The overall success of the baryonic scaling model suggests that the well-known global coupling between the baryonic mass of a galaxy and its rotation velocity (known as the baryonic Tully–Fisher relation) applies at a more local level as well, and it seems to imply a link between the baryonic mass distribution and the distribution of total mass (including dark matter). Optical and X-ray observations of candidate isolated neutron stars in the G315.4-2.3 supernova remnant

Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society 2012 RAS

Journal keyword(s): galaxies: dwarf - galaxies: kinematics and dynamics - galaxies: spiral

Simbad objects: 47

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2012MNRAS.425.2299S and select 'bookmark this link' or equivalent in the popup menu


2020.11.23-18:55:22

© Université de Strasbourg/CNRS

    • Contact