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Cloud Disruption and Formation

Published online by Cambridge University Press:  07 August 2017

Jan Palouš
Jan Palouš*
Affiliation:
Astronomical Institute of the Czechoslovak, Academy of Sciences, Budečská 6, 120 23 Prague 2, Czechoslovakia

Extract

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Star formation is responsible at least for a part of radiation coming from central regions of active galaxies. Violent bursts of star formation yield rapidly evolving massive stars, which transform in metal-rich enviroments into so called Warmers / Terlevich et al., 1987 / changing nebular spectra to Seyfert or Liner type.

Type
Part 5: Structure of the Central Object and NLR
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 314 - 315
Copyright
Copyright © Kluwer 1989 

References

Baan, W.A., van Gorkom, J., Schmelz, J.T., Mirabel, I.F. 1987 The Astrophys.J. 313, 102 Google Scholar
Bodenheimer, P., Tenorio-Tagle, G. 1988 Ann.Rew.Astron.Astrophys., in press Google Scholar
Franco, J., Palouš, J., Tenorio-Tagle, G. 1988, in preparation Mirabel, I.F., Sanders, D.B. 1988 The Astrophys.J. in press Google Scholar
Tenorio-Tagle, G., Palouš, J. 1987 Astron.Astrophys. 186, 287 Google Scholar
Terlevich, R., Melnick, J., Moles, M. 1987, in Observational Evidence of Activity in Galaxies /Eds Khachikian, E. Ye., Fricke, K.J., Melnick, J./, p.499 Google Scholar