Abstract
Stars having remarkable emission lines in the optical spectra are called emission-line stars and widely distributed on the Hertzsprung-Russell (HR) diagram including various stellar types:
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(1)
Early type stars—Wolf-Rayet (WR) stars, Of, Oe/Be/Ae stars, Luminous Blue Variables (LBV).
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(2)
Late type stars—dMe stars, flare stars, red giants, Mira variables.
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(3)
Close binaries—Algol stars, cataclysmic variables (CV), symbiotic stars.
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(4)
Pre-main sequence stars—Herbig Be/Ae stars, T Tauri stars.
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Further reading
Hearnshaw, J. B. (1986). The Analysis of Starlight, One Hundred and Fifty Years of Astronomical Spectroscopy. Cambridge University Press, Cambridge.
Leverington, D. (1995). A History of Astronomy from 1890 to the Present. Springer-Verlag, Berlin.
Tassoul, J.-L. and Tassoul, M. (2004). A Concise History of Solar and Stellar Physics. Princeton University Press, Princeton, NJ.
References
Beals, C. S. (1929). On the nature of Wolf-Rayet emission. MNRAS, 90, 202–212.
Bowen, I. S. (1928). The origin of the nebular lines and the structure of the planetary nebulae. Ap. J. 67, 1–15.
Burgers, J. M. and van de Hulst, H. C. (1951). Problems of cosmical aerodynamics. Proceedings of the Symposium on the Motion of Gaseous Masses of Cosmical Dimensions, Paris, August 16–19, 1949.
Cannon, A. J. (1916). Spectra having bright lines. Ann. Harvard Coll. Obs. 76, 19–42.
Deutsch, A. J. and Merrill, P. W. (1959). Gross differences between the R Cygni spectra at two successive maxima. Ap. J. 130, 570–577.
Henyey, L. G. (1938). The theory of cyclic transitions. Ap. J. 88, 133–163.
Herbig, G. H. (1952). Emission-line stars in galactic nebulosities. JRAS. Canada, 46, 222–233.
Herbig, G. H. (1958). Stars of F, G, and K with emission lines: Introductory report. Etoiles a raies d’emission. Liège Conference, July 1957, 251–270.
Herbig, G. H. (1960). The spectra of Be and Ae type stars associated with nebulosity. Ap. J. Suppl. 4, 337–368.
Hertzsprung, E. (1924). Note on a peculiar star or nova of short duration. Bull. Astr. Inst. 2, 87–88.
Joy, A. H. (1945). T Tauri variable stars. Ap. J. 102, 168–195.
Joy, A. H. (1948). Emission lines in stellar spectra. Ap. J. 53, 107.
Joy, A. H. and Humason, M. L. (1949). Observations of the faint dwarf star L726-8. PAS. Pacific, 61, 133–134.
Menzel, D. H. (ed.) (1962). Selected Papers on Physical Processes in Ionized Plasmas, Dover, New York.
Menzel, D. H. (ed.) (1966) Selected Papers on the Transfer of Radiation. Dover, NY.
Merrill, P. W. (1933). Four stars whose spectra have bright helium lines. Ap. J. 77, 44–50.
Merrill, P. W. (1958). Symbiosis in astronomy: Introductory report. Etoiles a raies d’emission. Liège Conference, July 1957, 436–448.
Miyamoto, S. (1943). On the envelopes of peculiar stars (in Japanese). Tenmongaku Iho 2, 157–186.
Miyamoto, S. (1953). The atmospheres of the P Cygni stars. PAS. Japan, 5, 55–73.
Parker, E. N. (1958). Dynamics of interplanetary gas and magnetic fields. Ap. J. 128, 664–676.
Pickering, E. C. (1890). The Draper Catalogue of stellar spectra photographed with the 8-inch Bache telescope as a part of Henry Draper Memorial. Harvard College Obs. Ann., 27, 1–388.
Pikel’ner, S. B. (1954). Spectrophotometric investigation on the mechanisms of excited filamentary nebulae. Izv. Krimk. Astrofiz. Obs. 12, 93.
Roques, P. (1955). A search for flare stars. PASP, 67, 34–38.
Rosseland, S. (1926). On the Origin of bright lines in stellar spectra. Ap. J., 63, 218–235.
Rosseland, S. (1936). Stars with extensive envelopes. Theoretical Astrophysics. Chapter 20. Oxford University Press, Oxford.
Schatzman, E. (1949). The heating of the solar corona and chromosphere. Ann. d’Ap., 12, 203–218.
Sobolev, V. V. (1847). Moving Envelopes of Stars (in Russian, English translation is published from Harvard Univ. Press in 1960).
Struve, O. (1931). On the origin of bright lines in spectra of stars of class B. Ap. J., 73, 94–103.
Struve, O. (1942). Extended stellar atmospheres: A review of the problems of gaseous shells. Ap. J., 95, 134–151.
van Maanen, A. (1940). The photographic determination of stellar parallaxes with the 60-and 100-inch telescopes Ap. J., 91, 503–506.
Wallerstein, G. (1959). The shock-wave model for the population II Cepheids. Ap. J., 130, 560–569.
Wilson, O. C. and Bappu, M. K. V. (1957). H and K emission in late type stars: Dependence of line width on luminosity and related topics. Ap. J., 125, 661–683.
Zanstra, H. (1927). An application of the quantum theory to the luminosity of diffuse nebulae. Ap. J., 65, 50–70.
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Kogure, T., Leung, KC. (2007). Introduction. In: The Astrophysics of Emission-Line Stars. Astrophysics and Space Science Library, vol 342. Springer, New York, NY. https://doi.org/10.1007/978-0-387-68995-1_1
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