Bibcode
Varela, A. M.; Beckman, J. E.; Cepa, J.; Muñoz-Tuñón, C.; Prieto, M.; Vilchez, J. M.
Bibliographical reference
International Conference on Dynamics and Interactions of Galaxies, p. 181 - 183
Advertised on:
0
1990
Citations
0
Refereed citations
0
Description
The authors show, in NGC 4736, that the bulge indicates strong and
radially variable ellipticity, evidence of star formation, and outflow,
while the bulge of the non-starburst galaxy NGC 5033 gives no evidence
of peculiar or variable ellipticity.