H I in the elliptical galaxy NGC 1052

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astronomical Spectroscopy, Elliptical Galaxies, Galactic Rotation, Hydrogen Atoms, Angular Resolution, Astronomical Maps, Centimeter Waves, Emission Spectra, High Resolution, Optical Emission Spectroscopy, Spiral Galaxies

Scientific paper

The E4 galaxy NGC 1052 has been mapped in the H I 21-cm emission line using the 100-m telescope. The H I associated with this galaxy is no more than about 4 arcmin in size. A systematic change in radial velocity is measured which suggests that the H I is a rotating system. The total amplitude of the observed rotation is about 100 km/s with an orientation of the dynamical major axis which is 54 (+ or - 10) deg from the major axis of the light distribution.

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