At the low-mass end - Light and H I distribution of GR 8

Astronomy and Astrophysics – Astronomy

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Astronomical Photometry, Dwarf Galaxies, Galactic Mass, H I Regions, Irregular Galaxies, Light Sources, Color-Magnitude Diagram, Dark Matter, Mass Distribution, Virgo Galactic Cluster

Scientific paper

The dwarf irregular galaxy GR 8, which is at the extreme faint end of the luminosity and mass functions, is studied using optical photometry and 21 cm H I line observations. For the light distribution, an exponential decline (as usual for more massive systems) is found with an extrapolated central surface brightness of B(O)c = 22.6 mag/sq arcsec and a scale length of 76 pc. The colors are typical of Im galaxies with (B - V) = 0.38. The H I is found to be clumpy with most of the gas just outside the optical image. Its radial distribution is well approximated by a Gaussian. From the kinematics, it is found that, contrary to what is normally observed, the rotation axis of the gas is parallel to the common major axis of the optical and H I distribution and not perpendicular. It is shown that rotation is only important to the gravitational support of the system in the inner parts (r less than 250 pc).

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