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The population of Magellanic Cloud planetary nebulae

Published online by Cambridge University Press:  01 July 2008

Letizia Stanghellini
Letizia Stanghellini*
Affiliation:
National Optical Astronomy Observatory, 950 N. Cherry Ave, Tucson AZ 85719, USA
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Abstract

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In this review we address the progress that has been made toward the understanding of Magellanic Cloud planetary nebulae (PNe) and their evolution since the last Magellanic Cloud Symposium. Planetary nebulae in the Magellanic Clouds are the key probes of stellar and circumstellar evolution, both for their known distances and relative vicinity, and for their broad metallicity range A selection of recent results is presented, including the HST study of PNe and their central stars, the study of the population of Magellanic Cloud PNe based on abundance analysis, the recent Spitzer analysis of their dust contents, and the use of Magellanic Cloud PNe to constrain the distance scale of Galactic PNe.

Keywords

stars: AGB and post-AGBstars: evolutionstars: windsoutflowsplanetary nebulae: generalMagellanic Clouds
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S256: The Magellanic System: Stars, Gas, and Galaxies , July 2008 , pp. 421 - 430
Copyright
Copyright © International Astronomical Union 2009

References

Acker, A., Marcout, J., Ochsenbein, F., Stenholm, B., & Tylenda, R. 1992, Strasbourg – ESO catalogue of galactic planetary nebulae (Garching: European Southern Observatory)Google Scholar
Bernard-Salas, J., Houck, J. R., Morris, P. W., Sloan, G. C., Pottasch, S. R., & Barry, D. J. 2004, ApJS, 154, 271CrossRefGoogle Scholar
Bernard-Salas, J., Pottasch, S. R., Gutenkunst, S., Morris, P. W., & Houck, J. R. 2008, ApJ, 672, 274Google Scholar
Cahn, J. H., Kaler, J. B., & Stanghellini, L. 1992, A&AS, 94, 399Google Scholar
Cioni, M.-R. L. & Habing, H. J. 2003, A&A, 402, 133Google Scholar
Costa, R. D. D., de Freitas Pacheco, J. A., & Idiart, T. P. 2000, A&AS, 145, 467Google Scholar
Daub, C. T. 1982, ApJ, 260, 612Google Scholar
Dopita, M. A. 1999, in Chu, Y.-H., Suntzeff, N., Hesser, J., & Bohlender, D. (eds.), New Views of the Magellanic Clouds, IAUS 190, p. 332Google Scholar
García-Segura, G. 1997, ApJ, 489, L189Google Scholar
Groenewegen, M. A. T., van Loon, J. T., Whitelock, P. A., Wood, P. R., & Zijlstra, A. A. 2000, in Wing, R. F. (ed.), The Carbon Star Phenomenon, IAUS 177 (Dordrecht: Kluwer), p. 385Google Scholar
Hora, J. L., Cohen, M., Ellis, R. G., et al. 2008, AJ, 135, 726Google Scholar
Idiart, T. P., Maciel, W. J., & Costa, R. D. D. 2007, A&A, 472, 101Google Scholar
Izzard, R. G., Dray, L. M., Karakas, A. I., Lugaro, M., & Tout, C. A. 2006, A&A, 460, 565Google Scholar
Jacoby, G. H. & De Marco, O. 2002, AJ, 123, 269CrossRefGoogle Scholar
Karakas, A. & Lattanzio, J. C. 2007, PASA, 24, 103CrossRefGoogle Scholar
Leisy, P. & Dennefeld, M. 2006, A&A, 456, 451Google Scholar
Leisy, P., Dennefeld, M., Alard, C., & Guibert, J. 1997, A&AS, 121, 407Google Scholar
Maraston, C. 2005, MNRAS, 362, 799Google Scholar
Marigo, P. 2001, A&A, 370, 194Google Scholar
Morris, M. 1981, ApJ, 249, 572Google Scholar
Reid, W. A. & Parker, Q. A. 2006, MNRAS, 373, 521CrossRefGoogle Scholar
Russell, S. C. & Bessell, M. S. 1989, ApJS, 70, 865Google Scholar
Shaw, R. A., Stanghellini, L., Mutchler, M., Balick, B., & Blades, J. C. 2001, ApJ, 548, 727Google Scholar
Shaw, R. A., Stanghellini, L., Villaver, E., & Mutchler, M. 2006, ApJS, 167, 201CrossRefGoogle Scholar
Soker, N. 1998, ApJ, 496, 833Google Scholar
Stanghellini, L., Shaw, R. A., Mutchler, M., Palen, S., Balick, B., & Blades, J. C. 2002, ApJ, 575, 178Google Scholar
Stanghellini, L., Shaw, R. A., Balick, B., Mutchler, M., Blades, J. C., & Villaver, E. 2003, ApJ, 596, 997Google Scholar
Stanghellini, L., Shaw, R. A., & Gilmore, D. 2005, ApJ, 622, 294Google Scholar
Stanghellini, L., Guerrero, M. A., Cunha, K., Manchado, A., & Villaver, E. 2006, ApJ, 651, 898Google Scholar
Stanghellini, L., García-Lario, P., García-Hernández, D. A., Perea-Calderón, J. V., Davies, J. E., Manchado, A., Villaver, E., & Shaw, R. A. 2007, ApJ, 671, 1669Google Scholar
Stanghellini, L., Shaw, R. A., & Villaver, E. 2008, ApJ, 689, 194CrossRefGoogle Scholar
Villaver, E., Stanghellini, L., & Shaw, R. A. 2003, ApJ, 597, 298CrossRefGoogle Scholar
Villaver, E., Stanghellini, L., & Shaw, R. A. 2004, ApJ, 614, 716Google Scholar
Villaver, E., Stanghellini, L., & Shaw, R. A. 2007, ApJ, 656, 831Google Scholar
Willson, L. A. 2000, ARAA, 38, 573Google Scholar