scholarly journals CCD photometry of Galactic clusters containing Cepheid variables - I. Lynga 6

1985 ◽  
Vol 213 (4) ◽  
pp. 889-897 ◽  
Author(s):  
A. R. Walker
Keyword(s):  
Ccd Photometry ◽  
Galactic Clusters ◽  
Cepheid Variables

Galactic Clusters with Associated Cepheid Variables. VI. Anonymous van den Bergh (C0634+031) and CV Monocerotis

1998 ◽  
Vol 115 (5) ◽  
pp. 1958-1971 ◽  
Author(s):  
David G. Turner ◽  
Mario H. Pedreros ◽  
Alistair R. Walker
Keyword(s):  
Galactic Clusters ◽  
Cepheid Variables

Cepheid Variables in the Large Magellanic Cloud Cluster NGC 1866. I. New BVRI CCD Photometry

2000 ◽  
Vol 129 (1) ◽  
pp. 111-121 ◽  
Author(s):  
Wolfgang P. Gieren ◽  
Matias Gomez ◽  
Jesper Storm ◽  
Thomas J. Moffett ◽  
L. Infante ◽  
...  
Keyword(s):  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Ccd Photometry ◽  
Cloud Cluster ◽  
Cepheid Variables

SPECTROSCOPIC INVESTIGATIONS OF GALACTIC CLUSTERS WITH ASSOCIATED CEPHEID VARIABLES. I. POLARIS CLUSTER AND α UMI

2018 ◽  
Vol 31 (0) ◽  
pp. 113-116
Author(s):  
I. A. Usenko ◽  
A. S. Miroshnichenko ◽  
S. Danford ◽  
V. V. Kovtyukh ◽  
D. G. Turner ◽  
...  
Keyword(s):  
Spectroscopic Investigations ◽  
Galactic Clusters ◽  
Cepheid Variables

scholarly journals SPECTROSCOPIC INVESTIGATIONS OF GALACTIC CLUSTERS WITH ASSOCIATED CEPHEID VARIABLES. III. COLLINDER 394 AND BB SGR

2019 ◽  
Vol 32 (0) ◽  
pp. 91-96
Author(s):  
I. A. Usenko ◽  
A. Yu. Kniazev ◽  
I. Yu. Katkov ◽  
V. V. Kovtyukh ◽  
T. V. Mishenina ◽  
...  
Keyword(s):  
Spectroscopic Investigations ◽  
Galactic Clusters ◽  
Cepheid Variables

scholarly journals 30. Commission des Vitesses Radiales Stellaires

1939 ◽  
Vol 6 ◽  
pp. 254-266 ◽  
Author(s):  
M. W. S. Adams ◽  
MM. Bok ◽  
Guthnick ◽  
Harper ◽  
Joy ◽  
...  
Keyword(s):  
Radial Velocities ◽  
Early Type ◽  
The Past ◽  
Special Groups ◽  
Mount Wilson Observatory ◽  
Galactic Clusters ◽  
Cepheid Variables ◽  
Early Type Stars ◽  
Large Telescopes ◽  
Selection Of

During the past three years the measurement of stellar radial velocities has formed an important part of the spectroscopic programme of most observatories possessing large telescopes. As observations are carried to fainter and fainter stars and the number of observable objects increases rapidly, a natural development has been the selection of special groups and types of stars, the radial velocities of which will aid in the solution of certain specific problems. Illustrations are the studies of the O, B and A type stars made at the Dominion Astrophysical, the Lick, and the Simeis Observatories, of the members of the galactic clusters at the Lick Observatory, and of the fainter Cepheid variables and early-type stars with strong interstellar lines at the Mount Wilson Observatory.

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