Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-13T03:55:00.865Z Has data issue: false hasContentIssue false

Spectrophotometry of 3C 232 and 3C 249.1

Published online by Cambridge University Press:  19 July 2016

D. Dultzin-Hacyan*
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado 70-264 México, D. F. 04510, MEXICO

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We find indication of variability of the ratio Mg II 2934/2798 for 3C 232 and discuss the excitation mechanism of Mg II 2934. For 3C 249.1 we identified the following new lines: [Ne V] 3346, [Ne V) 3426 and He I 3884. Comments are made on continuum shapes; in both cases optical continuum variability is confirmed.

Type
III. Spectral Line Studies
Copyright
Copyright © Reidel 1986 

References

Dultzin-Hacyan, D., Salas, L. and Daltabuit, E., 1982, Astr. and Ap., 111, 43.Google Scholar
Dultzin-Hacyan, D., 1985, Rev., Mex. Astron. y Astrof., 11, in press.Google Scholar
Firmani, C. and Ruíz, E., 1981, Recent Advances in Observational Astronomy, eds.: Johnson, H. L. and Allen, C. (México: UNAM), p. 25.Google Scholar
Grandi, S. A. and Phillips, M. N., 1978, Ap. J., 220, 426.Google Scholar