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Stellar Content of the Giant HII Region NGC 604
Published online by Cambridge University Press: 03 August 2017
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BVRI CCD frames of NGC 604, the brightest Hll region in the nearby spiral galaxy M33, have been obtained at the Nordic Optical Telescope (Canaries Islands). The seeing was 0.6″ which corresponds to ~ 2 pc. at the distance of M33. The magnitude of the stars were obtained using the Capella stellar photometry package (Debray et ai., 1989).
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- Session VI. Enrichment
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- Copyright © Kluwer 1991
References
Benvenuti, P., d'Odorico, S., Dumontel, M. (1979) Astrophysics and Space Science
66, 39
Google Scholar
Conti, P.S. (1986) in IAU Symposium 116, Luminous Stars and Associations in Galaxies, pp.199–214
Google Scholar
Debray, B., Llebaria, A., Dubout-Crillon, R., Petit, M. (1989) Proceedings of the 1st ESO/ST-ECF Data Analysis Workshop, Grosb⊘l, P., Murtagh, F. and Warmels, R. H.. (Eds.), 189
Google Scholar
D'Odorico, S., Rosa, M. (1981)
Proceedings of the ESO Workshop on “The Most Massive Stars”
, 191
Google Scholar
Israel, F.P., Hawarden, T.G., Geballe, T.R., Wade, R. (1990) Monthly Notices Roy. Astron. Soc.
242, 471
CrossRefGoogle Scholar
Madore, B.F., McAlary, C.W., McLaren, R.A., Welch, D.L., Neugebauer, G., Matthews, K. (1985) Astrophys. Journal
294, 560
CrossRefGoogle Scholar
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