Hostname: page-component-848d4c4894-hfldf Total loading time: 0 Render date: 2024-05-12T09:41:35.380Z Has data issue: false hasContentIssue false
  • English
  • Français

CCD photometry of HII galaxies

Published online by Cambridge University Press:  07 August 2017

Eduardo Telles ,
Roberto Terlevich  and
Bernard E.J. Pagel
Eduardo Telles
Affiliation:
Institute of Astronomy - Cambridge, UK
Roberto Terlevich
Affiliation:
Royal Greenwich Observatory - Cambridge, UK
Bernard E.J. Pagel
Affiliation:
NORDITA - Copenhagen, Denmark

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.

We report the first results of a multicolour (broad V,R,I and narrow [OIII] bands) surface photometry study of a small sample of HII galaxies.

The data were obtained at the 2.5m Nordic Optical Telescope (NOT) at La Palma, Canary Islands under subarcsecond seeing conditions. Part of the data has 0.55 arc seconds resolution (FWHM). The data will allow us to investigate the bi-parametric behaviour of the luminosity vs line-witdh relation.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 493
Copyright
Copyright © Kluwer 

References

Dressler, et al.: 1987, “, Astrophys. J. , 42.Google Scholar
Melnick, J., Moles, M., Terlevich, R. & Garcia-Pelayo, J.M.: 1987, “, Mon. Not. R. astr. Soc. , 849.CrossRefGoogle Scholar
Melnick, J., Terlevich, R. & Moles, M.: 1988, “, Mon. Not. R. astr. Soc. , 297.CrossRefGoogle Scholar
Terlevich, R. & Melnick, J.: 1981, “, Mon. Not. R. astr. Soc. , 839.CrossRefGoogle Scholar