Zobrazeno 1 - 10
of 16
pro vyhledávání: '"G. Siegfried Kutter"'
Publikováno v:
Physics of Classical Novae ISBN: 9783540535003
The nova outburst requires an energy source that is energetic enough to eject material and is able to recur. The Thermonuclear Runaway (TNR) model, coupled with the binary nature of nova systems satisfies these conditions. The white dwarf/red dwarf b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9ccd4a13a9576b644b56a00508d4fe25
https://doi.org/10.1007/3-540-53500-4_148
https://doi.org/10.1007/3-540-53500-4_148
Publikováno v:
International Astronomical Union Colloquium. 122:361-372
The nova outburst requires an energy source that is energetic enough to eject material and is able to recur. The Thermonuclear Runaway (TNR) model, coupled with the binary nature of nova systems, satisfies these conditions. The white dwarf/red dwarf
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8c17e4cfbba3e873c43b5329a93087b6
https://doi.org/10.1017/s0252921100068858
https://doi.org/10.1017/s0252921100068858
Autor:
G. Siegfried Kutter, Warren M. Sparks
Publikováno v:
Atmospheric Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion ISBN: 3540194789
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::61c58e3578f6af13703755f4910cd710
https://doi.org/10.1007/bfb0034604
https://doi.org/10.1007/bfb0034604
Autor:
Matthias Krodel, G. Siegfried Kutter
Publikováno v:
SPIE Proceedings.
Cesic -- a trademark of ECM for carbon-fiber reinforced silicon carbide -- allows relatively quick and cheap manufacturing of components because the components can be shaped with conventional tools in a milling and/or drilling process of the greenbod
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3d4344b1422940cfca8c4b795293ae9a
https://doi.org/10.1117/12.503771
https://doi.org/10.1117/12.503771
Autor:
Eric Ruch, G. Siegfried Kutter, Wilhelm Pfrang, Martin A. Seilonen, Gregory V. Mehle, Douglas C. Neam, Renaud Mercier-Ythier, Paul A. Lightsey, Brian E. Catanzaro, Scott Streetman, Claus Mueller, Ulrich Papenburg
Publikováno v:
SPIE Proceedings.
Challenges in high-resolution space telescopes have led to the desire to create large primary mirror apertures. One such telescope is the Next Generation Space Telescope (NGST, 8-m primary). In order to accommodate launch vehicles, the optical system
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2f8895b5fbfba5903ff6cf14b367e10c
https://doi.org/10.1117/12.394004
https://doi.org/10.1117/12.394004
Autor:
Warren M. Sparks, G. Siegfried Kutter
Publikováno v:
Cataclysmic Variables and Low-Mass X-Ray Binaries ISBN: 9789401088497
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2b07f340b2c863a587b99c4c84038e62
https://doi.org/10.1007/978-94-009-5319-2_50
https://doi.org/10.1007/978-94-009-5319-2_50
Autor:
G. Siegfried Kutter
Publikováno v:
Nature. 410:301-302
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f4f722a7c8f939848365b3e7852ee4f3
https://doi.org/10.1038/35066617
https://doi.org/10.1038/35066617
Autor:
G. Siegfried Kutter, Warren M. Sparks
Publikováno v:
International Astronomical Union Colloquium. 53:290-293
We assume that the outburst of classical novae is the result of transfer of H-rich material from a red secondary star to a He or C/O white dwarf and the development of a thermonuclear runaway in the e-degenerate “base of the accreted H-rich envelop
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::600f560f2d8ae38f66a8fc65a600eb9b
https://doi.org/10.1017/s0252921100076077
https://doi.org/10.1017/s0252921100076077
Autor:
Warren M. Sparks, G. Siegfried Kutter
Publikováno v:
International Astronomical Union Colloquium. 58:643-648
The rapid coherent oscillation during a dwarf nova outburst is attributed to an accretion-driven wave going around the white dwarf component of the binary system. The increase and decrease in the period of this oscillation is due to the change in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::420690919c5d82fd2d1183905a681810
https://doi.org/10.1017/s025292110008218x
https://doi.org/10.1017/s025292110008218x
Publikováno v:
Highlights of Astronomy. 5:505-508
The mass and energy of nova ejecta are 10-5 - 10-4M⊚ and 1044 - 1045 ergs, respectively (Payne-Gaposchkin 1957). Comparison of these quantities with the mass (1 M⊚) and binding energy (1051 erg) of the erupting white dwarf implies that the nova o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::28307b564b722a1cad147a2616bc37b3
https://doi.org/10.1017/s1539299600004378
https://doi.org/10.1017/s1539299600004378