Internal Motions in NGC 5128

Details Internal Motions in NGC 5128 Internal Motions in NGC 5128

Oct 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.224..253s&link_type=abstract

Nature, Volume 224, Issue 5216, pp. 253-254 (1969).

Astronomy and Astrophysics

Astrophysics

20

Scientific paper

DURING the past 2 years, NGC 5128 has been observed with various techniques at the 154 cm reflector in Bosque Alegre (Astrophysical Branch of the Observatorio de Córdoba). The aim of these observations was to measure the radial velocity field for emission and absorption lines in this galaxy in order to find whether there is relative motion between gas and stars as represented by the emission and absorption lines respectively. Previous work on this subject1-3 has given no definite results because of the difficulty of getting well exposed spectra simultaneously showing emission and absorption lines with moderate dispersion. Here I present some results.

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