Tight LMC massive star clusters R 127 and R 128

Free access article

Issue		A&A Volume 400, Number 3, March IV 2003


Page(s)		923 - 937
Section		Stellar clusters and associations
DOI		http://dx.doi.org/10.1051/0004-6361:20030066

Abstract : Tight LMC massive star R 128

References

Ardeberg, A., Brunet, J. P., Maurice, E., & Prevot, L. 1972, A&AS, 6, 249 NASA ADS
Clampin, M., Nota, A., Golimowski, D. A., Leitherer, C., & Durrance, S. T. 1993, ApJ, 410, L35 NASA ADS
Davies, R., Eliott, K., & Meaburn, J. 1976, Mem. R. Astron. Soc., 81, 89 NASA ADS
Feast, M. W., Thackeray, A. D., & Wesselink, A. J. 1960, MNRAS, 121, 337 NASA ADS
Fitzpatrick, E. L. 1988, ApJ, 335, 703 NASA ADS
Fitzpatrick, E. L. 1991, PASP, 103, 1123 NASA ADS
Fitzpatrick, E. L., & Garmany, C. D. 1990, ApJ, 363, 119 NASA ADS
Gallagher, J. S. 1989, in ASSL 157, IAU Colloq. 113, Physics of Luminous Blue Variables, ed. K. Davidson, A. Moffat, & H. Lamers, 185
Henize, K. G. 1956, ApJS, 2, 315 NASA ADS
Heydari-Malayeri, M., Courbin, F., Rauw, G., Esslinger, O., & Magain, P. 1997, A&A, 326, 143 NASA ADS
Humphreys, R. M., & Davidson, K. 1994, PASP, 106, 1025 NASA ADS
Isserstedt, J. 1975, A&AS, 19, 259 NASA ADS
Kaltcheva, N., & Georgiev, L. 1992, MNRAS, 259, 166 NASA ADS
Kukarkin, B., Kholopov, P., & Efremov, Y. N. 1974, Sec. Suppl. Third Edition Gen. Cat. Var. Stars, Nauka, Moscow, 10
Lamers, H. J. G. L. M., Bastiaanse, M. V., Aerts, C., & Spoon, H. W. W. 1998, A&A, 335, 605 NASA ADS
Lamers, H. J. G. L. M., Nota, A., Panagia, N., Smith, L. J., & Langer, N. 2001, ApJ, 551, 764 NASA ADS
Langer, N., Hamann, W.-R., Lennon, M., et al. 1994, A&A, 290, 819 NASA ADS
Lucke, P. B., & Hodge, P. W. 1970, AJ, 75, 171 NASA ADS
Maeder, A. 1997, in ASP Conf. Ser., ed. A. Nota & H. Lamers, 120, 374
Magain, P., Courbin, F., & Sohy, S. 1998, ApJ, 494, 472 NASA ADS
Manfroid, J., Sterken, C., Bruch, A., et al. 1991, A&AS, 87, 481 NASA ADS
Manfroid, J., Sterken, C., Cunow, B., et al. 1994, A&AS, 109, 329 NASA ADS
Martins, F., Schaerer, D., & Hillier, D. J. 2002, A&A, 382, 999 NASA ADS
Massey, P., & Johnson, J. 1993, AJ, 105, 980 NASA ADS
Meynet, G., Maeder, A., Schaller, G., Schaerer, D., & Charbonnel, C. 1994, A&AS, 103, 97 NASA ADS
Nota, A., & Clampin, M. 1997, in Luminous Blue Variables, Massive Stars in Transition, ed. A. Nota, & H. Lamers, ASP Conf. Ser., 120, 303
Nota, A., & Lamers, H. 1997, in ASP Conf. Ser., ed. A. Nota, & H. Lamers, 120
Nota, A., Leitherer, C., Clampin, M., & Gilmozzi, R. 1991, in Wolf-Rayet Stars and Interrelations with Other Massive Stars in Galaxies, ed. K. van der Hucht, & B. Hidayat, IAU Symp., 143, 561
Parker, J. W. 1997, in Luminous Blue Variables: Massive Stars in Transition, ed. A. Nota, & H. Lamers, ASP Conf. Ser., 120, 368
Parker, J. W., Garmany, C. D., Massey, P., & Walborn, N. R. 1992, AJ, 103, 1205 NASA ADS
Relyea, L. J., & Kurucz, R. L. 1978, ApJS, 37, 45 NASA ADS
Sanduleak, N. 1970, Cerro Tololo Inter-American Obs. Cont., 89
Schulte-Ladbeck, R. E., Leitherer, C., Clayton, G. C., et al. 1993, ApJ, 407, 723 NASA ADS
Shannon, C. 1949, Proc. I. R. E., 37, 10
Smith, L. J., Nota, A., Pasquali, A., et al. 1998, ApJ, 503, 278 NASA ADS
Spoon, H. W. W., de Koter, A., Sterken, C., Lamers, H. J. G. L. M., & Stahl, O. 1994, A&AS, 106, 141 NASA ADS
St-Louis, N., Turbide, L., & Moffat, A. 1997, in Luminous Blue Variables: Massive Stars in Transition, ed. A. Nota, & H. Lamers, ASP Conf. Ser., 120, 187
Stahl, O. 1987, A&A, 182, 229 NASA ADS
Stahl, O., Leitherer, C., Wolf, B., & Zickgraf, F.-J. 1984, A&A, 131, L5 NASA ADS
Stahl, O., Wolf, B., Klare, G., et al. 1983, A&A, 127, 49 NASA ADS
Sterken, C. 1983, The Messenger, 33, 10 NASA ADS
Sterken, C., Manfroid, J., Anton, K., et al. 1993, A&AS, 102, 79 NASA ADS
Sterken, C., Manfroid, J., Beele, D., et al. 1995, A&AS, 113, 31 NASA ADS
Tutukov, A. V., & Yungelson, L. R. 1980, Soviet Astron. Lett., 6, 271 NASA ADS
Vacca, W. D., Garmany, C. D., & Shull, J. M. 1996, ApJ, 460, 914 NASA ADS
van Genderen, A. M. 2001, A&A, 366, 508 NASA ADS
van Genderen, A. M., de Groot, M., & Sterken, C. 1997, A&AS, 124, 517 NASA ADS
van Genderen, A. M., Sterken, C., de Groot, M., & Reijns, R. A. 1998, A&A, 332, 857 NASA ADS
Walborn, N. R. 1977, ApJ, 215, 53 NASA ADS
Walborn, N. R. 1982, ApJ, 256, 452 NASA ADS
Walborn, N. R., & Blades, J. C. 1997, ApJS, 112, 457 NASA ADS
Walborn, N. R., Drissen, L., Parker, J. W., et al. 1999, AJ, 118, 1684 NASA ADS
Walborn, N. R., Evans, I. N., Fitzpatrick, E. L., & Phillips, M. M. 1991, in Wolf-Rayet Stars and Interrelations with Other Massive Stars in Galaxies, ed. K. van der Hucht, & B. Hidayat, IAU Symp., 143, 505
Walborn, N. R., & Fitzpatrick, E. L. 1990, PASP, 102, 379 NASA ADS
Walborn, N. R., Lennon, D. J., Heap, S. R., et al. 2000, PASP, 112, 1243 NASA ADS
Werner, K., & Rauch, T. 2001, in Eta Carinae and Other Mysterious Stars: The Hidden Opportunities of Emission Spectroscopy, ed. T. Gull, S. Johannson, & K. Davidson, ASP Conf. Ser., 242, 229
Whitelock, P. A., van Leeuwen, F., & Feast, M. W. 1997, in ESA SP-402: Hipparcos - Venice '97, 402, 213
Wolf, B. 1989, A&A, 217, 87 NASA ADS
Wolf, B., Stahl, O., Smolinski, J., & Casatella, A. 1988, A&AS, 74, 239 NASA ADS

Abstract : Tight LMC massive star R 128

What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.

If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.