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Spectroscopic Study of NGC 6119 - NGC 6120 System

Published online by Cambridge University Press:  25 May 2016

C. Surace ,
J. Hecquet  and
M. Auriere
C. Surace
Affiliation:
Observatoire de Marseille, 2, place Le Verrier, 13248 Marseille cedex 4 (France)
J. Hecquet
Affiliation:
Observatoire Midi Pyrennées, 14, Avenue E. Belin 31400 Toulouse (France)
M. Auriere
Affiliation:
Observatoire Midi Pyrennées, 14, Avenue E. Belin 31400 Toulouse (France)

Extract

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NGC6119 and NGC6120 have been listed in Kiso catalog (Takase et al., 1987) as Sc and Irr galaxies. They have been selected by their clumpy features in order to investigate their nature and star formation history using slit spectroscopy. They have similar systemic velocities (respectively 9215 and 9200 km ·s–1) and seem to be members of a low gravitational interacting system of 4 galaxies (with MCG-6-36-30 and NGC6122).

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 448
Copyright
Copyright © Kluwer 1996 

References

Maehara, H., Hamabe, H., Bottinelli, L., Gouguenheim, L., Takase, B., 1988, PASJ, 40, 47 Google Scholar
Mass Hess, J.M., Kunth, D., 1991, A&AS, 88, 399 Google Scholar
Takase, B., Miyauchi-Isobe, N., 1987, ATAO 2nd series, 21, 251 Google Scholar