Abstract
The globular cluster NGC 4590 has been observed at Haute Provence Observatory (photographic photometry, 80-cm reflector, F/6) and at the European Southern Observatory (image-tube, 152-cm reflector, F/15).
-
A sequence of red magnitudes, m r (λ eff ≅6400 Å) has been established around the cluster. It comprises 28 stars with magnitudes between 11.66 and 16.50.
-
Five new variable stars were discovered in a one square degree field, centered on the cluster.
-
Four other variable stars (No. 39, 40, 41, and 42) were discovered in the cluster.
Observations made in Part at Haute Provence Observatory (C.N.R.S.).
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
References
Agt, S. L. Th. J. van and Oosterhoff, P. Th.: 1959, Ann. Sterrew. Leiden, 21, 253.
Hogg, H. S.: 1972.: Publ. David Dunlap Obs. 3, No. 6
Rosino, L. and Pietra, S.: 1954, Publ. Oss. astr. Univ. Bologna,6 No. 5.
Sawyer, H. B.: 1939, Publ. David Dunlap Obs. 1 No. 4
Sawyer, H. B.: 1955, Publ. David Dunlap Obs. 2, No. 2
Shapley, H.: 1919, Publ. Astron. Soc. Pacific 31, 266.
Terzan, A.: 1965, Ann. Astrophys. 28, 935.
Yoss, K. M.: 1955, Astron. J. 60, 338.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1973 D. Reidel Publishing Company, Dordrecht, Holland
About this paper
Cite this paper
Terzan, A., Rutily, B., Ounnas, C. (1973). Variable Stars in NGC 4590. In: Fernie, J.D. (eds) Variable Stars in Globular Clusters and in Related Systems. Astrophysics and Space Science Library, vol 36. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2590-4_10
Download citation
DOI: https://doi.org/10.1007/978-94-010-2590-4_10
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-2592-8
Online ISBN: 978-94-010-2590-4
eBook Packages: Springer Book Archive