Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-25T18:22:42.606Z Has data issue: false hasContentIssue false

The Kinematics and Ages of Stars in Gliese’s Catalogue

Published online by Cambridge University Press:  30 March 2016

R. Wielen*
Affiliation:
Astronomisches Rechen-Institut, Heidelberg, F.R.G.

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.

This contribution gives some results on the kinematics and ages of stars near the Sun. These results are mainly based on the catalogue of nearby stars compiled by Gliese (1957, 1969 and minor recent modifications). Table I shows the number of objects under consideration. While the old catalogue (1957) contained only stars with distances r up to 20 pc, the new edition (1969) includes many stars with slightly larger distances. In Table I, a ‘system’ is either a single star or a binary or a multiple system. The number of systems with known space velocities nearer than 20 pc has increased by about 30% from 1957 to 1969. The first edition of Gliese’s catalogue (1957) has been analyzed in detail by Gliese (1956) and von Hoerner (1960).

Type
Joint Discussions
Copyright
Copyright © Reidel 1974

References

Arakelian, M. A.: 1968, Astrofizika 4, 617.Google Scholar
Barbanis, B. and Woltjer, L.: 1967, Astrophys. J. 150, 461.Google Scholar
Delhaye, J.: 1965, Stars and Stellar Systems 5, 61.Google Scholar
Eggen, O. J.: 1965, Stars and Stellar Systems 5, 111.Google Scholar
Gliese, W.: 1956, Z. Astrophys. 39, 1.Google Scholar
Gliese, W.: 1957, Mitt. Astron. Rechen-Inst. Heidelberg Serie A No. 8.Google Scholar
Gliese, W.: 1969, Veröffentl. Astron. Rechen-Inst. Heidelberg No. 22.Google Scholar
Gliese, W.: 1971, in Luyten, W. J. (ed.), ‘White Dwarfs’, IAU Symp. 42, 35.Google Scholar
Hoerner S., von: 1960, Fortschritte der Physik 8, 191.Google Scholar
Jahreiss, H.: 1974, unpublished Thesis, Heidelberg University.Google Scholar
Luyten, W. J.: 1968, Monthly Notices Roy. Astron. Soc. 139, 221.Google Scholar
Luyten, W. J.: 1974, this volume, p. 389.Google Scholar
Mayor, M.: 1972, Astron. Astrophys. 18, 97.Google Scholar
Mazzitelli, I.: 1972, Astrophys. Space Sci. 17, 378.CrossRefGoogle Scholar
McCuskey, S. W.: 1966, Vistas in Astronomy 7, 141.CrossRefGoogle Scholar
Murray, C. A. and Sanduleak, N.: 1971, Monthly Notices Roy. Astron. Soc. 155, 463.Google Scholar
Oort, J. H.: 1965, Stars and Stellar Systems 5, 455.Google Scholar
Spitzer, L. and Schwarzschild, M.: 1953, Astrophys. J. 118, 106.CrossRefGoogle Scholar
Vandervoort, P. O.: 1970, Astrophys. J. 162, 453.CrossRefGoogle Scholar
Vyssotsky, A. N.: 1963, Stars and Stellar Systems 3, 192.Google Scholar
Weistrop, D.: 1972, Astron. J. 77, 849.Google Scholar
Wilson, O. C.: 1964, Publ. Astron. Soc. Pacific 76, 28.Google Scholar
Wilson, O. C.: 1966, Science 151, 1487.Google Scholar
Wilson, O. and Woolley, R.: 1970, Monthly Notices Roy. Astron. Soc. 148, 463.Google Scholar
Woolley, R.: 1970, in Becker, W. and Contopoulos, G. (ed.), ‘The Spiral Structure of Our Galaxy’, IAU Symp. 38, 423.Google Scholar
Woolley, R., Pocock, S. B.., Epps, E. A., and Flinn, R.: 1971, Roy. Obs. Bull. No. 166.Google Scholar