Abstract
The results of spectroscopic observations of 30 galaxies from the Second Byurakan Spectral Sky Survey in a field of 16 square degrees centered at coordinates a = 15h30m, δ = + 53°are presented. The spectra were obtained on the 6-m telescope of the Special Astrophysical Observatory, Russian Academy of Sciences, in the wavelength range of 4000–7400 Å with 15 Å resolution. Emission lines are present in the spectra of most of the galaxies. Redshifts and absolute stellar magnitudes were determined for all the galaxies.
Similar content being viewed by others
Literature Cited
B. A. Markarian and D. A. Stepanian,Astrofizika,19, 639 (1983).
S. A. Hakopian and S. K. Balayan, “Instability phenomena and their role in the evolution of cosmic objects,” in: Proceedings of Symposium, Armenia [in Russian], in press.
V. L. Afanasiev, A. N. Burenkov, V. V. Vlasyuk, and S. U. Drabek, SAO Tech. Rep., No. 234 (1995).
V. V. Vlasyuk,Bull. Spec. Astrophys. Obs.,36, 107 (1993).
J. A. Stepanian, V. A. Lipovetskii (Lipovetsky), L. K. Erastova, A. I. Shapovalova, and S. A. Hakopian,Astrofiz. Issled. (Izv. SAO),35, 24 (1993).
J. A. Stepanian, V. A. Lipovetskii (Lipovetsky), L. K. Erastova, S. A. Hakopian, Yu. I. Izotov, and N. G. Guseva,Astrofiz. Issled. (Izv. SAO),35, 38 (1993).
Author information
Authors and Affiliations
Additional information
Translated from Astrofizika, Vol. 40, No. 2, pp. 169–175, April–June, 1997.
Rights and permissions
About this article
Cite this article
Akopian, S.A., Balayan, S.K. Investigation of galaxies in the second byurakan sky survey. I. Spectroscopic observations in a field at 15h30m, +59°. Astrophysics 40, 114–118 (1997). https://doi.org/10.1007/BF03036103
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/BF03036103