Zobrazeno 1 - 10
of 176
pro vyhledávání: '"Miller, T. B."'
Autor:
Cramer, William J., Noble, A. G., Rudnick, G., Pigarelli, A., Wilson, G., Bahé, Y. M., Cooper, M. C., Demarco, R., Matharu, J., Miller, T. B., Muzzin, A., Nantais, J., Sportsman, W., van Kampen, E., Webb, T. M. A., Yee, H. K. C.
The changes in colors across a galaxy are intimately connected to the galaxy's formation, growth, quenching history, and dust content. A particularly important epoch in the growth of galaxies is near $z \sim 2$ often referred to as `cosmic noon', whe
Externí odkaz:
http://arxiv.org/abs/2404.07355
Autor:
Spilker, J. S., Aravena, M., Bethermin, M., Chapman, S. C., Chen, C. -C., Cunningham, D. J. M., De Breuck, C., Dong, C., Gonzalez, A. H., Hayward, C. C., Hezaveh, Y. D., Litke, K. C., Ma, J., Malkan, M., Marrone, D. P., Miller, T. B., Morningstar, W. R., Narayanan, D., Phadke, K. A., Sreevani, J., Stark, A. A., Vieira, J. D., Weiss, A.
Galaxies grow inefficiently, with only a few percent of the available gas converted into stars each free-fall time. Feedback processes, such as outflowing winds driven by radiation pressure, supernovae or supermassive black hole accretion, can act to
Externí odkaz:
http://arxiv.org/abs/1809.01676
Autor:
Miller, T. B., Chapman, S. C., Aravena, M., Ashby, M. L. N., Hayward, C. C., Vieira, J. D., Weiß, A., Babul, A., Béthermin, M., Bradford, C. M., Brodwin, M., Carlstrom, J. E., Chen, Chian-Chou, Cunningham, D. J. M., De Breuck, C., Gonzalez, A. H., Greve, T. R., Harnett, J., Hezaveh, Y., Lacaille, K., Litke, K. C., Ma, J., Malkan, M., Marrone, D. P., Morningstar, W., Murphy, E. J., Narayanan, D., Pass, E., Perry, R., Phadke, K. A., Rennehan, D., Rotermund, K. M., Simpson, J., Spilker, J. S., Sreevani, J., Stark, A. A., Strandet, M. L., Strom, A. L.
Massive galaxy clusters are now found as early as 3 billion years after the Big Bang, containing stars that formed at even earlier epochs. The high-redshift progenitors of these galaxy clusters, termed 'protoclusters', are identified in cosmological
Externí odkaz:
http://arxiv.org/abs/1804.09231
Autor:
Marrone, D. P., Spilker, J. S., Hayward, C. C., Vieira, J. D., Aravena, M., Ashby, M. L. N., Bayliss, M. B., Bethermin, M., Brodwin, M., Bothwell, M. S., Carlstrom, J. E., Chapman, S. C., Chen, Chian-Chou, Crawford, T. M., Cunningham, D. J. M., De Breuck, C., Fassnacht, C. D., Gonzalez, A. H., Greve, T. R., Hezaveh, Y. D., Lacaille, K., Litke, K. C., Lower, S., Ma, J., Malkan, M., Miller, T. B., Morningstar, W. R., Murphy, E. J., Narayanan, D., Phadke, K. A., Rotermund, K. M., Sreevani, J., Stalder, B., Stark, A. A., Strandet, M. L., Tang, M., Weiss, A.
According to the current understanding of cosmic structure formation, the precursors of the most massive structures in the Universe began to form shortly after the Big Bang, in regions corresponding to the largest fluctuations in the cosmic density f
Externí odkaz:
http://arxiv.org/abs/1712.03020
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America, 1967 Aug . 58(2), 513-517.
Externí odkaz:
https://www.jstor.org/stable/58239
Autor:
Miller, T. B.
Publikováno v:
The Journal of Modern History, 1960 Mar 01. 32(1), 1-15.
Externí odkaz:
https://www.jstor.org/stable/1871821
Akademický článek
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Publikováno v:
AFIPS Joint Computer Conferences; May1963, p127-140, 14p
Publikováno v:
Animal Production; 06/01/1978, Vol. 26 Issue 3, p339-342, 4p