Zobrazeno 1 - 10
of 998
pro vyhledávání: '"Ott U"'
Publikováno v:
Clinical Ophthalmology, Vol Volume 17, Pp 385-390 (2023)
Ursula Schmidt-Ott,1 Scott Fitzpatrick,2 Zoran Hasanbasic,3 Sergio Leal,3 Peter Morgan-Warren,4 Xin Zhang,3 Kristian T Johnson5 1Bayer AG, Berlin, Germany; 2Bayer AG, Mississauga, Canada; 3Bayer Consumer Care AG, Basel, Switzerland; 4Bayer PLC, Readi
Externí odkaz:
https://doaj.org/article/b7fd7202cd4d45ec9ca17768b36c9dc9
Publikováno v:
Progress in Particle and Nuclear Physics Volume 102, September 2018, Pages 1-47
In addition to long-lived radioactive nuclei like U and Th isotopes, which have been used to measure the age of the Galaxy, also radioactive nuclei with half-lives between 0.1 and 100 million years (short-lived radionuclides, SLRs) were present in th
Externí odkaz:
http://arxiv.org/abs/1808.00233
Publikováno v:
AIP Conference Proceedings 1595, 62 (2014)
Still today, the nucleosynthesis origin of Xe-H in presolar nanodiamonds is far from understood. Historically, possible explanations were proposed by a secondary "neutron-burst" process occurring in the He- or C/O-shells of a type-II supernova (SN-II
Externí odkaz:
http://arxiv.org/abs/1406.0725
Publikováno v:
Publ.Astron.Soc.Austral.26:297-302,2009
Knowledge about the age of presolar grains provides important insights into Galactic chemical evolution and the dynamics of grain formation and destruction processes in the Galaxy. Determination from the abundance of cosmic ray interaction products i
Externí odkaz:
http://arxiv.org/abs/0909.5532
Publikováno v:
In Geochimica et Cosmochimica Acta 15 August 2018 235:153-172
Publikováno v:
Astron.Astrophys. 426 (2004) 219-227
The J=2-1 and 3-2 rotational lines of the rare isotopomer C36S and the J=5-4 and 6-5 transitions of Si36S were detected in the carbon star IRC+10216 (CW Leo). These are the first detections of 36S bearing molecules in a star and the first spectroscop
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407003
Proceedings of "Nuclei in the Cosmos 2000", Aarhus, Danmark
Comment: 3 pages, 2 figures; to be publ. in Nucl. Phys. A
Comment: 3 pages, 2 figures; to be publ. in Nucl. Phys. A
Externí odkaz:
http://arxiv.org/abs/astro-ph/0012280
Autor:
Andersen, A. C., Jager, C., Mutschke, H., Braatz, A., Clement, C., Henning, Th., Jorgensen, U. G., Ott, U.
Publikováno v:
1999, A&A 343, 933
We present here the first infrared spectra of meteoritic SiC grains. The mid-infrared transmission spectra of meteoritic SiC grains isolated from the Murchison meteorite were measured in the wavelength range 2.5--16.5 micron, in order to make availab
Externí odkaz:
http://arxiv.org/abs/astro-ph/9812401
Akademický článek
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Autor:
Wallner, A., Melber, K., Merchel, S., Ott, U., Forstner, O., Golser, R., Kutschera, W., Priller, A., Steier, P.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, B January 2013 294:496-502