Hostname: page-component-848d4c4894-wg55d Total loading time: 0 Render date: 2024-04-30T16:39:14.196Z Has data issue: false hasContentIssue false

The Stellar Population in Galaxies Observed on the Astrophysical Station “ASTRON”

Published online by Cambridge University Press:  07 August 2017

I. Pronik
Affiliation:
Crimean Astrophysical Observatory, USSR
N. Merkulova
Affiliation:
Crimean Astrophysical Observatory, USSR
L. Metik
Affiliation:
Crimean Astrophysical Observatory, USSR
V. Pronik
Affiliation:
Crimean Astrophysical Observatory, USSR

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.

25 star systems were observed in 1983-1987 with the 80cm telescope on the board of astrophysical station “Astron”. Entrance diaphragms were 60″ and 10″. Spectrometer with the exit slit 28 A has measured fluxes in erg/sec cm2 A in the region 1600-3500 AA in regime of narrow band photometry. Exposures in every point were 2-5 min for bright objects and 10-30 min for week ones.

Type
III. The Stellar Populations of Non-Resolved Galaxies
Copyright
Copyright © Kluwer 

References

Aiello, S., Barsella, B., Chlewicki, G., Greenberg, J., Patriachi, P., Perinotto, M. (1988), Astron.Astrophys. , V. 73, P.195.Google Scholar
Bergh van den, S.(1960), Publ.David Dunlap Obs. , V. 11, No 6.Google Scholar
Brusual, G.A. (1983), Astrophys.J. , V. 273, P. 105.CrossRefGoogle Scholar
Burstein, D., Bertola, F., Buson, L., Faber, S., Lauer, T., (1988), Astrophys.J. , V. 328, P.440.CrossRefGoogle Scholar
Ciani, A., D'Odorico, S., Benvenuti, P. (1984), Astron.Astrophys. , V. 137, P.223.Google Scholar
Faber, S. (1983), Highlights of Astronomy , V. 6, P.165.CrossRefGoogle Scholar
Faber, S., Burstein, D., Dressler, A. (1977), Astron.J. , V. 82, P.941.CrossRefGoogle Scholar
Jamar, C., Macau, D. (1974), Astron.Astrophys. , V. 33, P.87.Google Scholar