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Flash stars in stellar aggregates

Published online by Cambridge University Press:  14 August 2015

Guillermo Haro
Guillermo Haro*
Affiliation:
Tonantzintla and Tacubaya Observatories

Extract

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In the past 10 years numerous extremely rapid variables have been found in different stellar associations. The spectrophotometric characteristics of some of these explosive variables are so similar to those of the UV Ceti stars that we propose the term “flash stars” for this variety, in order to provisionally distinguish them from the classical flare stars.

Type
Section 1: The Galaxy
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 30 - 37
Copyright
Copyright © Australian Academy of Science 1964 

References

Ambartsumian, V. A. (1954).—Soob. Byurakan. Obs. No. 13.Google Scholar
Ambartsumian, V. A. (1957).—“Non-stable Stars.” (Ed. Herbig, G. H..) Symp. IAU 3: 177–85. [Dublin 1955.] (Cambridge Univ. Press.)Google Scholar
Dall'almo, U. (1958).— Coelum 25: No. 1–2.Google Scholar
Haro, G. (1953).— Ap. J. 117: 73–82.CrossRefGoogle Scholar
Haro, G. (1954a).—Ton. y Tac., Bol. No. 11: 11–18.Google Scholar
Haro, G. (1954b).—Personal communication to Rosino and Herbig.Google Scholar
Haro, G. (1957).—“Non-stable Stars.” (Ed. Herbig, G. H..) Symp. IAU 3: 26–30. [Dublin 1955.] (Cambridge Univ. Press.)Google Scholar
Haro, G. (1962).—“Symposium on Stellar Evolution.” pp. 37–44. [La Plata Observatory 1960.] (Nat. Univ. La Plata Astron. Obs.)Google Scholar
Haro, G., and Chavira, E. (1955).—Ton. y Tac, Bol. No. 12: 3–16.Google Scholar
Haro, G., and Chavira, E. (1963).—Still unpublished.Google Scholar
Haro, G., Chavira, E., and Mendoza, E. (1960).— A.J. 65: 490.Google Scholar
Haro, G., and Morgan, W. W. (1953).— Ap. J. 118: 16–17.Google Scholar
Haro, G., and Rivera Terrazas, L. (1954).—Ton. y Tac, Bol. No. 10: 3–15.Google Scholar
Herbig, G. H. (1962).— Ap. J. 135: 736–47.Google Scholar
Johnson, H. L., and Mitchell, R. I. (1958).— Ap. J. 128: 31–40.Google Scholar
Joy, A. H. (1949).— Ap. J. 110: 424–37.Google Scholar
Joy, A. H. (1960).—“Stars and Stellar Systems.” (General Ed. Kuiper, G. P..) vol. VI. pp. 653–75. (Univ. Chicago Press.)Google Scholar
Oskanjan, V. (1957a).—“Non-stable Stars.” pp. 17–27. [Byurakan 1956.] (Acad. Sci. Armenian SSR: Erevan.)Google Scholar
Oskanjan, V. (1957b). —Personal communication.Google Scholar
Petit, M. (1958).—“Colloqui d'Astrofisica di Asiago (1956–1958).” Asiago Contr. No. 95: 29–44.Google Scholar
Rosino, L. (1956).—Asiago Contr. No. 69.Google Scholar
Rosino, L., and Cian, A. (1962).—Asiago Contr. No. 125.Google Scholar
Rosino, L., Grubissich, C., and Maffei, P. (1957).—Asiago Contr. No. 82.Google Scholar