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Ultraviolet Observations of Be Stars: (Review Paper)

Published online by Cambridge University Press:  14 August 2015

Sara R. Heap
Sara R. Heap*
Affiliation:
Laboratory for Optical Astronomy, NASA Goddard Space Flight Center, Greenbelt, Md., U.S.A.

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The history of ultraviolet studies of Be stars is barely ten years old. However, in the last decade, twelve major space experiments have observed Be stars in the ultraviolet region of the spectrum, and ultraviolet data for over 30 Be stars are now available in the literature. Table I shows some of the characteristics of the experiments. They include two rockets, five astronomical satellites, three manned satellites, and one planetary probe. Except for the rocket experiments, they are primarily survey instruments, which have provided ultraviolet data on early-type stars in general, and these data have proved to be extremely useful as standards of comparison for Be stars. Of the twelve spacecraft, two are presently operating: Copernicus and ANS. The two experiments complement one another very nicely in that the ANS experiment can obtain absolute continuous flux distributions, while the Princeton experiment can obtain high-resolution line spectra for the brighter Be stars.

Type
Part III: New Observational Techniques
Information
Symposium - International Astronomical Union , Volume 70: Be and Shell Stars , 1976 , pp. 165 - 178
Copyright
Copyright © Reidel 1976 

References

Beeckmans, F.: 1975, Astron. Astrophys. , in press.Google Scholar
Bless, R. C. and Code, A. D.: 1972, Ann. Rev. Astron. Astrophys. 10, 197.Google Scholar
Bohlin, R.: 1970, Astrophys. J. 162, 571.Google Scholar
Bohlin, R.: 1975, Astrophys. J. 200, 402.Google Scholar
Boksenberg, A., Evans, R. G., Fowler, R. G., Gardner, I. S. K., Houziaux, L., Humphries, C. M., Jamar, C., Macau, D., Macau, J. P., Malaise, D., Monfils, A., Nandy, K., Thompson, G. I., Wilson, R., and Wroe, H.: 1973, Monthly Notices Roy. Astron. Soc. 163, 291.Google Scholar
Bottemiller, R.: 1972, in Code, A. D. (ed.), Symposium on Scientific Results from OAO-2 , Amherst, p. 505.Google Scholar
Burton, W. and Evans, R. G.: 1976, this volume, p. 199.Google Scholar
Code, A. D., Houck, T. E., McNall, J. F., Bless, R. C., and Lillie, C. F.: 1970, Astrophys. J. 161, 377.Google Scholar
Collins, G. W.: 1974a, Astrophys. J. 191, 157.Google Scholar
Collins, G. W.: 1974b, private communication.Google Scholar
Coyne, G.: 1972, in Code, A. D. (ed.), Symposium on Scientific Results from OAO-2 , Amherst, p. 495.Google Scholar
Davis, R. J., Deutschman, W. A., Lundquist, C. A., Nozawa, Y., and Bass, S. B.: 1972, in Code, A. D. (ed.), Symposium on Scientific Results from OAO-2 , Amherst, p. 495.Google Scholar
Delplace, A. M. and Van der Hucht, K. A.: 1976, this volume, p. 197.Google Scholar
Gurzadyan, G. A., Kashin, A. L., Krmoyan, M. N., and Ohanesyan, J. B.: 1974, Astrofizika 10, 177.Google Scholar
Heap, S. R.: 1975, Phil. Trans. Roy. Soc. London A. 279, 371.Google Scholar
Heap, S. R. and Stecher, T. P.: 1974, Astrophys. J. 187, L27.Google Scholar
Henry, R. C., Weinstein, A., Feldman, P. D., Fastie, W. G., and Moos, H. W.: 1975, Astrophys. J. , in press.Google Scholar
Henize, K. G., Wray, J. D., Parsons, S. B., and Benedict, G. F.: 1976, this volume, p. 191.Google Scholar
de Jager, C. Hoekstra, R., Van der Hucht, K. A., Kamperman, T. M., Lamers, H. J., Hammerschlag, A., Werner, W., and Emming, J. G.: 1974, Astrophys. Space Sci. 26, 207.Google Scholar
Kelly, R. and Palumbo, L. J.: 1973, Atomic and Ionic Emission Lines Below 2000 Angstroms , NRL Report 7599, Naval Research Lab., Washington, D.C. Google Scholar
Kondo, Y., Modisette, J. L., and Wolf, G. W.: 1975, Astrophys. J. 199, 100.Google Scholar
Lamars, H. J. G. L. M. and Snijders, M. A. J.: 1975, Astron. Astrophys. 41, 259.Google Scholar
Lillie, C. F., Bohlin, R. C., Molnar, M. R., Barth, C. A., and Lane, A. L.: 1972, Science 175, 321.Google Scholar
Marlborough, J. M. and Snow, T. P.: 1976, this volume, p. 179.Google Scholar
Marlborough, J. M. and Zamir, M.: 1975, Astrophys. J. 195, 145.Google Scholar
Mihalas, D. M.: 1972, Non-LTE Model Atmospheres for B and O Stars , NCAR-TN/STR-76, NCAR, Boulder, Colorado.Google Scholar
Molnar, M. R.: 1975, Astrophys. J. 200, 106.Google Scholar
Paczynski, B.: 1971, Acta Astron. 23, 191.Google Scholar
Panek, R. J. and Savage, B. D.: 1976, Astrophys. J. , in press.Google Scholar
Peters, G.: 1976, this volume, p. 209.Google Scholar
Rogerson, J. B., Spitzer, L., Drake, J. F., Dressler, K. Jenkins, E. B., Morton, D. C., and York, D. G.: 1973, Astrophys. J. 181, L97.Google Scholar
Schild, R. 1973: Astrophys. J. 179, 221.CrossRefGoogle Scholar
Slettebak, A.: 1949, Astrophys. J. 110, 498.Google Scholar
Slettebak, A.: 1966, Astrophys. J. 145, 126.Google Scholar
Smith, A. M.: 1967, Astrophys. J. 147, 158.Google Scholar
Snow, T. P.: 1975, Astrophys. J. 198, 361.Google Scholar
Thompson, G. I., Humphries, C. M., and Nandy, K.: 1974, Astrophys. J. 187, L81.Google Scholar
Underhill, A. B.: 1952, Publ. Dominion Astrophys. Obs. 9, 139.Google Scholar
Underhill, A. B., Leckrone, D. S., and West, D. K.: 1972, Astrophys. J. 171, 63.Google Scholar
Underhill, A. B. and Van der Hucht, K. A.: 1975, submitted to Astron. Astrophys. Google Scholar
Van Duinen, R. J., Aalders, J. W. G., and Wesselius, P. R.: 1973, ‘Announcement of Opportunity’, Dept. of Space Research, Groningen.Google Scholar
Viotti, R.: 1975, ‘Ultraviolet Energy Distribution of the B3e Star HD 200775 in NGC 7023 From TD1-S2/68 Observations’, submitted to Astron. Astrophys. Google Scholar