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Titlebook: Mathematical Methods for Objects Reconstruction; From 3D Vision to 3D Emiliano Cristiani,Maurizio Falcone ?,Silvia Tozza Conference proceed

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發(fā)表于 2025-3-25 06:32:47 | 只看該作者
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發(fā)表于 2025-3-25 08:14:00 | 只看該作者
Conference proceedings 2023uture scientific leaders in the field of 3D data acquisition, 3Dscene reconstruction, and 3D printing software development will find an excellent introduction to these problems and to the mathematical techniques necessary to solve them..
23#
發(fā)表于 2025-3-25 12:01:25 | 只看該作者
24#
發(fā)表于 2025-3-25 18:52:22 | 只看該作者
Emiliano Cristiani,Maurizio Falcone,Silvia TozzaeppoSAX added important information on the pulsar emission in the harder band pass whereas EUVE and HST allowed to study neutron stars in the very soft 0.07—0.2 keV and optical/UV bands. More details on results from observations of neutron stars can be found in the Chaps. 6—8. New excellent observat
25#
發(fā)表于 2025-3-25 20:06:33 | 只看該作者
Georg Radow,Giuseppe Rodriguez,Ashkan Mansouri Yarahmadi,Michael Breu?he hot wind equation for the pair plasma and the relativistic Grad-Schlüter-Shafranov (GSS) equation for the magnetic flux function. The structure of the solutions for the hot pair wind equation is discussed. We also show how self-consistent axisymmetric MHD magnetospheres can be constructed by simu
26#
發(fā)表于 2025-3-26 03:14:59 | 只看該作者
Toby Collins,Adrien Bartoliics and astrophysics of neutron stars and black holes is here attacked from both theoretical and experimental points of view. In the experimental field we range from the reviews and catalogues of galactic X-ray sources (R. Gursky and E. Schreier) and pulsars (E. Groth) to the observations of the opt
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發(fā)表于 2025-3-26 06:08:02 | 只看該作者
28#
發(fā)表于 2025-3-26 11:05:25 | 只看該作者
Jesse Beisegel,Johannes Buhl,Rameez Israr,Johannes Schmidt,Markus Bambach,Armin Fügenschuhlsar can continue to vaporize the low-mass companion star even after the accretion turn-off produced by a strong pulsar wind; (5) the RD-evolutionary model resolves the apparent statistical discrepancy between the number of MSP’s and their LMXB progenitors.
29#
發(fā)表于 2025-3-26 16:37:24 | 只看該作者
30#
發(fā)表于 2025-3-26 20:30:51 | 只看該作者
2281-518X 3D printing software development will find an excellent introduction to these problems and to the mathematical techniques necessary to solve them..978-981-99-0778-6978-981-99-0776-2Series ISSN 2281-518X Series E-ISSN 2281-5198
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