... GAIA-C5-TN-UB-JMC-011 Hamuy, M., Suntzeff, N. B., Heathcote, S. R., Walker, A. R., Gigoux, P., & Phillips, M. M. 1994, PASP, 106, 566 Hamuy, M., Walker, A. R., Suntzeff, N. B., Gigoux, P., Heathcote, S. R., & Phillips, M. M. 1992, PASP, 104, 533 Kaiser, M ...
... M SNe (%) 23 56 M Winds (%) 77 44 Total MHe (M yr-1 ) 0.26 0.43 T MOotal (M yr-1 ) 0.04 0.04 Total Mass (M ) 2.3 в 106 3.7 в 106 7 7 Starbursts are important sources for energizing and enriching the ISM and -- via galactic superwinds -- possibly the IGM ...
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Ссылки http://www.stsci.edu/science/starburst/Preprints/moriond99.pdf -- 128.4 Кб -- 12.08.2003 Похожие документы
... AK06) Anthony-Twarog B. J., Twarog, B. A., & Sheeran, M. 1994, PASP, 106, 486 Campins, H., Rieke, G. H., & Leb ofsky, M. J. 1985, AJ, 90, 896 Cohen, M., Walker, R. G., Carter, B., Hammersley, P. Kidger, M. & Noguchi, K. 1999, AJ, 117, 1864 de Jager, C ...
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Ссылки http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-000959.pdf -- 350.7 Кб -- 05.02.2013 Похожие документы
... By scaling the luminosity of a 7 Myr star cluster of 106M (MV = -15.5 according to STARBURST99 models), we find that any young clusters which are not observed in the archival WFPC2 images would have masses of several hundred solar masses and less (i.e ...
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Ссылки http://www.stsci.edu/science/starburst/Preprints/Chandar_Diffuse.pdf -- 780.0 Кб -- 31.03.2005 Похожие документы
... L17 Hamuy, M., Suntze, N. B., Heathcote, S. R., Walker, A. R., Gigoux, P., & Schechter, P. 1976, ApJ, 203, 297 Phillips, M. M. 1994, PASP, 106, 566 Schlegel, D. J., Finkbeiner, D. P., & Davis, M. 1997, ApJ, 500, 525 Hobbs, L. M. 1974a, ApJ, 191, 381 Silva ...
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Ссылки http://www.stsci.edu/~mutchler/documents/ApJ_1999_GRB97.pdf -- 176.1 Кб -- 31.10.2002 Похожие документы
... Star-formation law: continuous. Star formation rate = 1 M yr -1 . M low = 1 M. ... 106 . Solid line: . = 2.35, M up = 100 M . Long-dashed line: . = 3.30, M up = 100 M . ...
... Star-formation law: continuous. Star formation rate = 1 M yr -1 . M low = 1 M. ... 106 . Solid line: . = 2.35, M up = 100 M . Long-dashed line: . = 3.30, M up = 100 M . ...