Zobrazeno 1 - 10
of 42
pro vyhledávání: '"SPARKS, W. M."'
Autor:
Starrfield, S., Timmes, F. X., Iliadis, C., Hix, W. R., Arnett, W. D., Meakin, C., Sparks, W. M.
Publikováno v:
Baltic Astronomy, Vol 21, pages 76 - 87, 2012
Symbiotic binaries are systems containing white dwarfs (WDs) and red giants. Symbiotic novae are those systems in which thermonuclear eruptions occur on the WD components. These are to be distinguished from events driven by accretion disk instabiliti
Externí odkaz:
http://arxiv.org/abs/1211.6145
Autor:
Starrfield, S., Iliadis, C., Timmes, F. X., Hix, W. R., Arnett, W. D., Meakin, C., Sparks, W. M.
We present a brief summary of the Single Degenerate Scenario for the progenitors of Type Ia Supernovae in which it is assumed that a low mass carbon-oxygen white dwarf is growing in mass as a result of accretion from a secondary star in a close binar
Externí odkaz:
http://arxiv.org/abs/1210.6086
Publikováno v:
Astrophys.J.692:1532-1542,2009
We have continued our studies of the Classical Nova outburst by evolving TNRs on 1.25Msun and 1.35Msun WDs (ONeMg composition) under conditions which produce mass ejection and a rapid increase in the emitted light, by examining the effects of changes
Externí odkaz:
http://arxiv.org/abs/0811.0197
Publikováno v:
AIP Conf.Proc.891:364-372,2007
Classical novae participate in the cycle of Galactic chemical evolution in which grains and metal enriched gas in their ejecta, supplementing those of supernovae, AGB stars, and Wolf-Rayet stars, are a source of heavy elements for the ISM. Once in th
Externí odkaz:
http://arxiv.org/abs/0706.0558
Publikováno v:
Astrophys.J. 612 (2004) L53-L56
Nova explosions occur on the white dwarf (WD) component of a Cataclysmic Variable stellar system which is accreting matter lost by a companion. A Type Ia supernova explosion is thought to result when a WD, in a similar binary configuration, grows in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407466
Autor:
Godon, P., Sion, E. M., Cheng, F., Gaensicke, B. T., Howell, S., Knigge, C., Sparks, W. M., Starrfield, S.
Publikováno v:
Astrophys.J. 602 (2004) 336-341
FUSE and HST/STIS spectra of the dwarf nova WZ Sge, obtained during and following the early superoutburst of July 2001 over a time span of 20 months, monitor changes in the components of the system during its different phases. The synthetic spectral
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310876
Autor:
Bender, R., Macchetto, F., Nieto, J. L., Caon, N., Davoust, E., Piotto, G., Poulain, P., Prieur, J. L., Prugniel, P., Rampazzo, R., Scorza, C., Sparks, W. M., Surma, P., Wagner, S., CAPACCIOLI, MASSIMO
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3730::66d2c8b735e17ad8098b433203e354c9
http://hdl.handle.net/11588/477837
http://hdl.handle.net/11588/477837
Akademický článek
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Publikováno v:
AIP Conference Proceedings; 2000, Vol. 522 Issue 1, p379, 4p, 2 Charts
Autor:
Starrfield, S., Timmes, F. X., Hix, W. R., Iliadis, C., Arnett, W. D., Meakin, C., Sparks, W. M.
Publikováno v:
Proceedings of the International Astronomical Union; Jul2011 Supplement, Vol. 7 Issue S281, p166-171, 6p