Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-25T05:25:15.860Z Has data issue: false hasContentIssue false
  • English
  • Français

A Decoupled Nucleus in NGC 1052

Published online by Cambridge University Press:  07 August 2017

O.K. Sil'chenko
O.K. Sil'chenko*
Affiliation:
Sternberg Astronomical Institute, University av. 13, Moscow 119899, Russia. E-mail: [email protected]

Extract

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.

The central part of NGC 1052 has been observed at the prime focus of the 6m telescope with the Multi-Pupil Spectrophotometer equipped with a two-dimensional IPCS. Ninety-nine spectra over the central 14.5″x11″ are registered in the spectral range of λλ4700 – 5400 AA and are used to map ionized-gas velocities (by [OIII]λ5007) and to derive radial profiles of absorption-line equivalent width for MgIλA5175, FeIλ5270, and Hβ.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 438
Copyright
Copyright © Kluwer 1995 

References

Bender, R. and Surma, P. (1992) Astron. Astrophys., 258, pp. 250–254 Google Scholar
Davies, R.L. and Illingworth, G.D. (1986) Astrophys. J., 302, pp. 234–244 Google Scholar
Sil'chenko, O.K., Afanasiev, V.L., Vlasiuk, V.V. (1992) Astron. Zh., 69, pp. 1121–1135 Google Scholar
Sparks, W.B., Wall, J.V., Jorden, P.R., Thorne, D.J., and Van Breda, I. (1991) Astrophys. J. Suppl. Ser., 76, pp. 471–524 Google Scholar
Worthey, G. (1992) , California Univ. Google Scholar