Zobrazeno 1 - 10
of 216
pro vyhledávání: '"Klaus Bernhard"'
Autor:
Daniele Buono, Gulzar Khan, Klaus Bernhard von Hagen, Petr A. Kosachev, Eike Mayland-Quellhorst, Sergei L. Mosyakin, Dirk C. Albach
Publikováno v:
Frontiers in Plant Science, Vol 11 (2021)
Climatic fluctuations in the Pleistocene caused glacial expansion-contraction cycles in Eurasia and other parts of the world. Consequences of these cycles, such as population expansion and subsequent subdivision, have been studied in many taxa at int
Externí odkaz:
https://doaj.org/article/140f63da1413420baa466ecdb6b4068e
Autor:
Ewa Niemczura, Stefan Hümmerich, Fiorella Castelli, Ernst Paunzen, Klaus Bernhard, Franz-Josef Hambsch, Krzysztof Hełminiak
Publikováno v:
Scientific Reports, Vol 7, Iss 1, Pp 1-11 (2017)
Abstract HD 66051 is an eclipsing system with an orbital period of about 4.75 d that exhibits out-of-eclipse variability with the same period. New multicolour photometric observations confirm the longevity of the secondary variations, which we interp
Externí odkaz:
https://doaj.org/article/667dc2bbee254db383324e8ea05d2b72
Autor:
Klaus Bernhard Bærentsen
Publikováno v:
Frontiers in Psychology, Vol 6 (2015)
Externí odkaz:
https://doaj.org/article/77691a70bcd348609312ef0166fdbc81
Akademický článek
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Publikováno v:
Plant Systematics and Evolution, 2016 Feb 01. 302(2), 155-172.
Externí odkaz:
https://www.jstor.org/stable/44852771
Shell stars, in particular the cooler ones, often do not show conspicuous Balmer-line emission and may consequently be missed in surveys that specifically search for emission signatures in the Halpha line. The present work is aimed at identifying sta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ff999e7905cf75c76d05be74203b27a
http://arxiv.org/abs/2210.14656
http://arxiv.org/abs/2210.14656
Autor:
Franz-Josef Hambsch, Klaus Bernhard, S. Otero, Stefan Hümmerich, Christopher Lloyd, Ernst Paunzen
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 499:3976-3991
According to most literature sources, the amplitude of the pulsational variability observed in γ Doradus stars does not exceed 0.1 mag in Johnson V. We have analysed fifteen high-amplitude γ Doradus stars with photometric peak-to-peak amplitudes we
Autor:
Hannah Stocker, Léon Beyer, Laura Perna, Ben Schöttker, Klaus Bernhard Gerwert, Hermann Brenner
Publikováno v:
Alzheimer's & Dementia. 17