Zobrazeno 1 - 10
of 186
pro vyhledávání: '"Young, T R"'
The first stars continue to elude modern telescopes, but much has been accomplished in observing the glow of the first galaxies. As detection capabilities improve we will eventually resolve these galaxies, but hopes of observing an individual star re
Externí odkaz:
http://arxiv.org/abs/1503.07231
We present stellar evolution calculations for Population III stars for both single and binary star evolution. Our models include 10 Msun and 16.5 Msun single stars and a 10 Msun model star that undergoes an episode of accretion resulting in a final m
Externí odkaz:
http://arxiv.org/abs/0710.3548
Autor:
Turatto, M., Suzuki, T., Mazzali, P. A., Benetti, S., Cappellaro, E., Danziger, I. J., Nomoto, K., Nakamura, T., Young, T. R., Patat, F.
The extraordinary SN 1997cy associated with GRB 970514 has been observed photometrically and spectroscopically for nearly 2 yr. At the time of discovery SN 1997cy was the brightest SN ever observed (Mv=<-20.1, v(hel)=19140 km/s, H_0=65 km/s/Mpc). Up
Externí odkaz:
http://arxiv.org/abs/astro-ph/9910324
Autor:
Iwamoto, K., Mazzali, P. A., Nomoto, K., Umeda, H., Nakamura, T., Patat, F., Danziger, I. J., Young, T. R., Suzuki, T., Shigeyama, T., Augusteijn, T., Doublier, V., Gonzalez, J. -F., Boehnhardt, H., Brewer, J., Hainaut, O. R., Lidman, C., Leibundgut, B., Cappellaro, E., Turatto, M., Galama, T. J., Vreeswijk, P. M., Kouveliotou, C., van Paradijs, J., Pian, E., Palazzi, E., Frontera, F.
Publikováno v:
Nature 395 (1998) 672-674
The discovery of the peculiar supernova (SN) 1998bw and its possible association with the gamma-ray burst (GRB) 980425$^{1,2,3}$ provide new clues to the understanding of the explosion mechanism of very massive stars and to the origin of some classes
Externí odkaz:
http://arxiv.org/abs/astro-ph/9806382
Autor:
Turatto, M., Mazzali, P. A., Young, T. R., Nomoto, K., Iwamoto, K., Benetti, S., Cappellaro, E., Danziger, I. J., de Mello, D. F., Phillips, M. M., Suntzeff, N. B., Clocchiatti, A., Piemonte, A., Leibundgut, B., Covarrubias, R., Maza, J., Sollerman, J.
SN 1997D in NGC 1536 is possibly the least luminous and energetic Type II supernova discovered to date. The entire light curve is subluminous, never reaching $M_V = -14.65$. The radioactive tail follows the 56Co decay slope. In the case of nearly com
Externí odkaz:
http://arxiv.org/abs/astro-ph/9803216
Rayleigh-Taylor (R-T) instabilities in the explosion of SN 1993J are investigated by means of two-dimensional hydrodynamical simulations. It is found that the extent of mixing is sensitive to the progenitor's core mass and the envelope mass. Because
Externí odkaz:
http://arxiv.org/abs/astro-ph/9701083
Autor:
Young, T. R.
Publikováno v:
Contemporary Sociology, 1999 May 01. 28(3), 268-270.
Externí odkaz:
https://www.jstor.org/stable/2654138
