scholarly journals Illuminating Endocrine Evolution: The Power and Potential of Large-Scale Comparative Analyses

2018 ◽  
Vol 58 (4) ◽  
pp. 712-719 ◽  
Author(s):  
Maren N Vitousek ◽  
Michele A Johnson ◽  
Jerry F Husak

2012 ◽  
Vol 35 (4) ◽  
pp. 238-239 ◽  
Author(s):  
Simon M. Reader ◽  
Steven M. Hrotic

AbstractEvolutionary questions require specialized approaches, part of which are comparisons between close relatives. However, to understand the origins of human tool behavior, comparisons with solely chimpanzees are insufficient, lacking the power to identify derived traits. Moreover, tool use is unlikely a unitary phenomenon. Large-scale comparative analyses provide an alternative and suggest that tool use co-evolves with a suite of cognitive traits.



2008 ◽  
Vol 64 (1) ◽  
pp. 86-97
Author(s):  
Go HAGIHARA ◽  
Toshimichi MURAO ◽  
Kazuyuki SHIMADA ◽  
Keiko YOSHIURA ◽  
Satoshi FUJII


2018 ◽  
Vol 58 (4) ◽  
pp. 720-728 ◽  
Author(s):  
Michele A Johnson ◽  
Clinton D Francis ◽  
Eliot T Miller ◽  
Cynthia J Downs ◽  
Maren N Vitousek


2012 ◽  
Vol 61 (6) ◽  
pp. 1017-1025 ◽  
Author(s):  
Arne Warth ◽  
Thomas Muley ◽  
Esther Herpel ◽  
Michael Meister ◽  
Felix J F Herth ◽  
...  


Cell ◽  
2020 ◽  
Vol 182 (5) ◽  
pp. 1328-1340.e13 ◽  
Author(s):  
Na Jia ◽  
Jinfeng Wang ◽  
Wenqiang Shi ◽  
Lifeng Du ◽  
Yi Sun ◽  
...  


2021 ◽  
Vol 12 ◽  
Author(s):  
Neng Wei ◽  
Oscar A. Pérez-Escobar ◽  
Paul M. Musili ◽  
Wei-Chang Huang ◽  
Jun-Bo Yang ◽  
...  

With c. 2,000 species, Euphorbia is one of the largest angiosperm genera, yet a lack of chloroplast genome (plastome) resources impedes a better understanding of its evolution. In this study, we assembled and annotated 28 plastomes from Euphorbiaceae, of which 15 were newly sequenced. Phylogenomic and comparative analyses of 22 plastome sequences from all four recognized subgenera within Euphorbia revealed that plastome length in Euphorbia is labile, presenting a range of variation c. 42 kb. Large-scale expansions of the inverted repeat (IR) region were identified, and at the extreme opposite, the near-complete loss of the IR region (with only 355 bp left) was detected for the first time in Euphorbiaceae. Other structural variations, including gene inversion and duplication, and gene loss/pseudogenization, were also observed. We screened the most promising molecular markers from both intergenic and coding regions for phylogeny-based utilities, and estimated maximum likelihood and Bayesian phylogenies from four datasets including whole plastome sequences. The monophyly of Euphorbia is supported, and its four subgenera are recovered in a successive sister relationship. Our study constitutes the first comprehensive investigation on the plastome structural variation in Euphorbia and it provides resources for phylogenetic research in the genus, facilitating further studies on its taxonomy, evolution, and conservation.



1999 ◽  
Vol 173 ◽  
pp. 243-248
Author(s):  
D. Kubáček ◽  
A. Galád ◽  
A. Pravda

AbstractUnusual short-period comet 29P/Schwassmann-Wachmann 1 inspired many observers to explain its unpredictable outbursts. In this paper large scale structures and features from the inner part of the coma in time periods around outbursts are studied. CCD images were taken at Whipple Observatory, Mt. Hopkins, in 1989 and at Astronomical Observatory, Modra, from 1995 to 1998. Photographic plates of the comet were taken at Harvard College Observatory, Oak Ridge, from 1974 to 1982. The latter were digitized at first to apply the same techniques of image processing for optimizing the visibility of features in the coma during outbursts. Outbursts and coma structures show various shapes.



1994 ◽  
Vol 144 ◽  
pp. 29-33
Author(s):  
P. Ambrož

AbstractThe large-scale coronal structures observed during the sporadically visible solar eclipses were compared with the numerically extrapolated field-line structures of coronal magnetic field. A characteristic relationship between the observed structures of coronal plasma and the magnetic field line configurations was determined. The long-term evolution of large scale coronal structures inferred from photospheric magnetic observations in the course of 11- and 22-year solar cycles is described.Some known parameters, such as the source surface radius, or coronal rotation rate are discussed and actually interpreted. A relation between the large-scale photospheric magnetic field evolution and the coronal structure rearrangement is demonstrated.



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