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Massive Stars and Giant HII Regions: The High-Energy Picture

Published online by Cambridge University Press:  03 August 2017

Thierry Montmerle
Thierry Montmerle*
Affiliation:
Service d'Astrophysique, Centre d'Etudes Nucléaires de Saclay 91191 Gif-sur-Yvette Cedex, France

Abstract

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Giant HII regions contain highly energetic objects: luminous, massive stars (including Wolf-Rayet stars) generating powerful winds, as well as, often, supernova remnants. These objects interact with the surrounding gas by creating shock waves. Part of the energy input is radiated away in the form of X-rays; also, protons and electrons may be accelerated in situ and generate γ-rays by collisions with the ionized gas. In addition, the stars themselves (including the accompanying low-mass PMS stars) are sources of X-rays, and W-R stars may emit continuum y-rays and are associated with nuclear γ-ray lines seen in the interstellar medium. Therefore, both through the stars they contain and through interactions within the gas, giant HII regions are, in addition to their more traditional properties and over nearly 7 decades in energy, important sources of high-energy radiation.

Type
Session VI. Enrichment
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 397 - 408
Copyright
Copyright © Kluwer 1991 

References

REFERENCES

Becker, R.H., Boldt, E.A., Holt, S.S., Pravdo, S.M., Rothschild, R.E., Serlemitsos, P.J., Swank, J.H. (1976), Ap.J. (Letters) 209, L65.CrossRefGoogle Scholar
Bertout, C. (1989), Ann. Rev. Astr. Ap. 27, 351.CrossRefGoogle Scholar
Bieging, J.H., Abbott, D.C., Churchwell, E.B. (1989), Ap.J. 340, 518.Google Scholar
Bignami, G.F., Hermsen, W. (1983), Ann. Rev. Astr. Ap. 21, 67.CrossRefGoogle Scholar
Bouvier, J. (1990), Astr. Ap., in press.Google Scholar
Breitschwerdt, D., Kahn, F.D. (1988), M.N.R.A.S. 235, 1011.CrossRefGoogle Scholar
Breitschwerdt, D., Kahn, F.D. (1989), M.N.R.A.S. 242, 209.Google Scholar
Campbell, P.M. (1984), Phys. Rev. A 30, 365.Google Scholar
Cesarsky, C.J., Montmerle, T. (1983), Sp. Sci. Rev. 36, 173.CrossRefGoogle Scholar
Chlebowski, T. (1989), Ap.J. 342, 1091.CrossRefGoogle Scholar
Chlebowski, T., Harnden, F.R. Jr., Sciortino, S. (1989), Ap.J. 341, 427.Google Scholar
Chlebowski, T., Seward, F.D., Swank, J., Szymkoviak, A. (1984), Ap.J. 281, 665.CrossRefGoogle Scholar
Chu, Y.-H. (1983), Ap.J 269, 202.CrossRefGoogle Scholar
Chu, Y.-H., Mac Low, M.-M. (1990), Ap.J., in press.Google Scholar
Dorland, H., Montmerle, T. (1987), Astr. Ap. 177, 243.Google Scholar
Dorland, H., Montmerle, T., Doom, C. (1986), Astr. Ap. 160, 1.Google Scholar
Drury, L. O'C. (1983), Rep. Progr. Phys. 46, 973.Google Scholar
Feigelson, E.D. (1987), in Proc. 5th Cambridge Cool Star Workshop, eds. Linsky, J.L. and Stencel, R. (Berlin: Springer), p. 455.Google Scholar
Gaetz, T.J., Salpeter, E.E. (1983), Ap. J. Suppl. 52, 155.Google Scholar
Hogg, D.E. (1989), Astr. J. 98, 282.Google Scholar
van der Hucht, K.A., Hidayat, B., Admiranto, A.G., Supelli, K.R., Doom, C. (1988), Astr. Ap. 199 217.Google Scholar
Koyama, K (1987), Pub.A.S.J. 41, 665.Google Scholar
Koyama, K., Asaoka, I., Ushimaru, N., Yamauchi, S., Corbet, R.H.D. (1990), Ap.J., in press.Google Scholar
Langer, N. (1989), Astr. Ap. 220, 135.Google Scholar
Luciani, J.F., Mora, P., Pellat, R. (1985), Phys. Fluids 28, 835.Google Scholar
Meaburn, J., Solomos, N., Laspias, V., Goudis, C. (1989), Astr. Ap. 225, 497.Google Scholar
Montmerle, T. (1979), Ap.J. 231, 95.Google Scholar
Montmerle, T. (1985), Proc. 19th Int. Cosmic Ray Conf., San Diego, 1, 209.Google Scholar
Montmerle, T. (1986), Proc. Advances in Nuclear Astrophysics, Paris, eds. Vangioni-Flam, E. et al. (Gif-sur-Yvette: Editions Frontières), p. 335.Google Scholar
Montmerle, T. (1987), Proc. Starbursts and Galaxy Evolution, Les Arcs, eds. Thuan, T.X., Montmerle, T., and Tran Than Van, J. (Gif-sur-Yvette: Editions Frontières), p. 47.Google Scholar
Montmerle, T. (1988), Proc. NATO ASI Genesis and Propagation of Cosmic Rays, Erice, eds. Shapiro, M.M. and Wefel, J.P. (Dordrecht: Reidel), p. 131.Google Scholar
Montmerle, T., André, Ph. (1988), Proc. NATO ASI Formation and Evolution of Low-Mass stars, Viana do Castelo, eds. Dupree, A.K. and Lago, M.T.V.T. (Dordrecht: Reidel), p. 225.CrossRefGoogle Scholar
Montmerle, T., Cesarsky, C.J. (1981), Proc. Int. School and Workshop Plasma Astrophysics , Varenna, ESA SP-161, 319.Google Scholar
Montmerle, T., Koch-Miramond, L., Falgarone, E., Grindlay, J. (1983), Ap.J. 269, 182.Google Scholar
Pollock, A.M.T. (1987a), Astr. Ap. 171, 135.Google Scholar
Pollock, A.M.T. (1987b), Ap.J. 320, 283.Google Scholar
Prantzos, N., Cassé, M. (1986), Ap.J. 307, 324.Google Scholar
Prantzos, N., Cassé, M., Arnould, M. (1988), Proc. 20th Int. Cosmic Ray Conf., Moscow, 1, 152.Google Scholar
Rosner, R., Golub, L., Vaiana, G.S. (1985), Ann. Rev. Astr. Ap. 23, 413.Google Scholar
Seward, F.D., Chlebowski, T. (1982), Ap.J. 256, 530.Google Scholar
Signore, M., Vedrenne, G. (1988), Astr. Ap. 201, 379.Google Scholar
Völk, H. (1988), Proc. 20th Int. Cosmic Ray Conf., Moscow, 7, 157.Google Scholar
Walter, R., Maeder, A. (1989), Astr. Ap. 218, 123.Google Scholar
Warwick, R.S., Norton, A.J., Turner, M.J.L., Watson, M.G., Willingale, R. (1988), M.N.R.A.S. 232, 551.Google Scholar
Warwick, R.S., Turner, M.J.L., Watson, M.G., Willingale, R. (1985), Nature 317, 218.CrossRefGoogle Scholar
Weaver, R., McCray, R., Castor, J., Shapiro, P., Moore, R. (1977), Ap.J. 218, 377.Google Scholar
Williams, P.M., van der Hucht, K.A., Pollock, A.M.T., Florkowski, D.R., van der Woerd, H., Wamsteker, W.M. (1990), M.N.R.A.S. 243, 662.Google Scholar