Hostname: page-component-848d4c4894-xm8r8 Total loading time: 0 Render date: 2024-06-23T04:51:44.003Z Has data issue: false hasContentIssue false
  • English
  • Français

32. Commission des ‘Selected Areas’

Published online by Cambridge University Press:  25 April 2016

P. J. van Rhijn

Abstract

An abstract is not available for this content so a preview has been provided. As you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Part III: Rapports et Comptes Rendus des Seances es Commissions
Information
Transactions of the International Astronomical Union , Volume 10 , 1960 , pp. 502 - 508
Copyright
Copyright © Cambridge University Press 1960

References

[1] Kooreman, C. J. and Oosterhoff, P. Th. Photographie magnitudes of 15651 stars brighter than 10·5 magnitude in the southern Selected Areas, derived from plates taken by DrWesselink, A. J.. Ann. Sternw. Leiden, 21, Tweede stuk, 1957.Google Scholar
[2] Pettit, E. Magnitudes and color indices of extra-galactic nebulae determined photo-electrically. Ap. J. 120, 416, 1954.CrossRefGoogle Scholar
[3] Yoss, K. M. Photo-red magnitude sequences in the north polar sequence and Selected Area 61. Astr. J. 60, 339, 1955. Google Scholar
[4] Tripp, W. Photographische Polarisationsmessungen und Dreifarbenphotometrie in Selected Area 40. Z. Ap. 41, 84, 1956.Google Scholar
[5] Rybka, E. Standard two-colour magnitudes of 38 stars near the Selected Areas 1 to 19. Acta Astr. 7, 65, 1957. Google Scholar
[6] Elvius, T. A photometric and spectrophotometric investigation.... Second Catalogue (812 stars in Selected Areas nos. 3, 4 and 5). Ann. Stockholm Obs. Bd. 18, no. 7, 1955 and Bd. 19, no. 3, 1956.Google Scholar
[7] Deutsch, A. N. Observations of variable stars in 74 Selected Areas north of declination + 15°. Variable Stars, Moscow 5, 225, 1939.Google Scholar
[8] Kurochkin, N. E. On 20 new variable stars in the region π2 Cyg and Selected Area 41. Variable Stars, Moscow 9, 197–204, 1953.Google Scholar
[9] Kurochkin, N. E. 16 new variable stars in Selected Area 9. Variable Stars, Moscow 9, 402–6, 1954.Google Scholar
[10] Kurochkin, N. E. Variable stars in Selected Area no. Variable Stars, Moscow 10, 171–4, 1955.Google Scholar
[11] Kurochkin, N. E. New variable stars in Selected Area 110. Variable Stars, Moscow 11, 111–15, 1956.Google Scholar
[12] van Rhijn, P. J. and Plaut, L. Proper motions of stars in the Selected Areas at the equator derived from plates taken at the Alger Observatory. Publ. Kapteyn Astr. Lab., Groningen, no. 56, 1955.Google Scholar
[13] Cape Mimeograms, no. 3, 1953.Google Scholar
[14] Ann. Sternw. Leiden, 19, Tweede stuk, 1946.Google Scholar
[15] Trans. I.A.U. 9, 468, 1957. Google Scholar
[16] Trans. I.A.U. 9, 465 and 466, 1957.Google Scholar
[17] Trans. I.A.U. 8, 479, 1952; and 9, 467, 1957.Google Scholar
[18] Trans. I.A.U. 7, 334, 1950. CrossRefGoogle Scholar
[19] Trans. I.A.U. 8, 485–95, 1952.Google Scholar
[20] Fehrenbach’s method has been described in J. d. Obs. 38, 165–87, 1955; and 39, 53 and 104, 1956.Google Scholar
[21] Publ. Obs. Haute Provence, 3, no. 38, 1955.Google Scholar
[22] Lodén, L. O. Arkiv. Astr. Bd. 2, no. 11, 1957.Google Scholar
[23] B.A.N. no. 473, 1956.Google Scholar
[24] Ann. Stockholm Obs. Bd. 19, no. 3, 1956.Google Scholar
[25] Groningen Publications, no. 57, 1955 and no. 59, 1956.Google Scholar
[26] Astr. J., Moscow, 33, 855, 1956; Astr. Obs. Warsaw Univ., Reprint no. 2, 1957.Google Scholar
[27] Smithson. Contr. Astrophys. 1, no. 1, 155, 1957; Sky and Telescope, 16, 214, 1957.Google Scholar
[28] Ap. J. 121, 161, 1955.Google Scholar
[29] Trans. I.A.U. 9, 475, 1957. Google Scholar