... M., Lagage P.O., Roth M., Testi L., 1997, ``Subнarcsec resolution images of the star forming region G 35.20-1.74'', A&A, 327, 299 [A14] Testi L., Felli M., Persi P., Roth M., 1998, ``HII and hot dust emission around young massive stars in G 9.62+0.19'', A ...
... E., & Krumm, N. 1983, ApJ, 267, 35 Giovanelli, R., Haynes, M. P., Kent, B. R., et al ... L27 Kewley, L. J., & Dopita, M. A. 2002, ApJS, 142, 35 Kewley, L. J., & Ellison, S ...
... Daytime visits (reserved for schools): every day from 10:00 to 12:00 p.m. Nighttime visits for groups of up to 35 people maximum takes place in the week of the first quarter moon: . ...
... Assume that the distribution of disk masses is a power law of the form N(m;m + dm) = km \Gammafi dm with fi = 2.35, following the Salpeter IMF. ...
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... 2003, PASP, 115, 928 Kewley, L. J., & Dopita, M. A. 2002, ApJS, 142, 35 Kewley, L. J., & Ellison, S. L. 2008, ApJ, 681, 1183 Kobulnicky, H. A., & Kewley, L. J. 2004, ApJ, 617, 240, KK04 Koda, J., & Sofue, Y. 2006, PASJ, 58, 299 Koornneef, J. 1982, A&A ...
... 1-3 2003 Global Science Forum Wavefront Control (P. Salinari) 35 OWL (European Southern Observatory, 100 m telescope study) A six mirror, spherical primary design with a 30 m flat segmented secondary that could become a high order corrector all other ...
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Ссылки http://www.arcetri.astro.it/~salinari/GSF/Wavefront%20Control.pdf -- 1770.4 Кб -- 27.11.2003 Похожие документы