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Photometric investigation of the association Car OB 2

Published online by Cambridge University Press:  14 August 2015

W. Seggewiss*
Affiliation:
Observatorium Hoher List der Universitäts-Sternwarte Bonn, Germany

Abstract

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A photometric investigation of the association Car OB 2 was carried out with a photoelectric standard sequence observed with the ESO photometric telescope and plates taken with the ADH telescope of Boyden Observatory. The distance of Car OB 2 is 2.04 kpc, the color excess EB–V is 0m.38. The main sequence of this ‘OB’ association reaches at least to late A-type stars. The luminosity function was determined and compared with the luminosity functions of very young open clusters observed by Walker (1957). The distance of a group of 13 early-type stars in the area of Car OB 2 (‘group c’) was found to be 2.5 kpc, the reddening 0m.68. The relation of Car OB 2 and group c to the structure of the Carina arm is regarded.

Type
Part II/Observations of Spiral Structure in Our Galaxy
Copyright
Copyright © Reidel 1970 

References

Beer, A.: 1961, Monthly Notices Roy. Astron. Soc. 123, 191.Google Scholar
Bok, B. J. and van Wijk, U.: 1952, Astron. J. 57, 213.Google Scholar
Feinstein, A.: 1964, Observatory 84, 111.Google Scholar
Hoffleit, D.: 1956, Astrophys. J. 124, 61.Google Scholar
Jaschek, M. and Jaschek, C.: 1959, Publ. Astron. Soc. Pacific 71, 465.Google Scholar
Salpeter, E. E.: 1955, Astrophys. J. 121, 161.Google Scholar
Schmidt, H. and Diaz Santanilla, G.: 1964, Veröffent. Astron. Inst. Univ. Bonn, 71.Google Scholar
Seggewiss, W.: 1968, Z. Astrophys. 68, 142.Google Scholar
Walker, M. F.: 1957, Astrophys. J. 125, 636.Google Scholar