scholarly journals Deciphering the period spacing pattern in the oscillation spectrum of the SPB star KIC 7760680

2017 ◽  
Vol 160 ◽  
pp. 03012
Author(s):  
Wojciech Szewczuk ◽  
Jadwiga Daszyńska-Daszkiewicz ◽  
Przemysław Walczak
Development ◽  
1996 ◽  
Vol 122 (3) ◽  
pp. 997-1005 ◽  
Author(s):  
J.C. Larkin ◽  
N. Young ◽  
M. Prigge ◽  
M.D. Marks

Arabidopsis trichomes are single-celled epidermal hairs that serve as a useful model for the study of plant cell differentiation. An examination of the distribution of trichomes early in their development revealed that developing trichomes occur adjacent to another trichome much less frequently than would be expected by chance. Clonal analysis of epidermal cell lineages ruled out a role for cell lineage in generating the observed minimum-distance spacing pattern. Taken together, these results are consistent with a role for lateral inhibition in the control of trichome development. We also report the identification of a new locus, Reduced Trichome Number (RTN), which affects the initiation of trichomes. This locus was initially detected by the reduced number of leaf trichomes on Landsberg erecta plants compared to that on Columbia plants. Quantitative Trait Locus mapping revealed that more than 73% of the variation in trichome number was due to a major locus near erecta on chromosome 2. The reduced number of trichomes conditioned by the Landsberg erecta allele of this locus appeared to be due to an early cessation of trichome initiation. The implications of these observations are discussed with regard to previously published models of trichome development.


2015 ◽  
Vol 11 (A29B) ◽  
pp. 567-572
Author(s):  
Jakub Ostrowski ◽  
Jadwiga Daszyńska-Daszkiewicz ◽  
Henryk Cugier

AbstractWe present the new interpretation of the oscillation spectrum of HD 163899 based on the new determinations of the effective temperature, mass-luminosity ratio and rotational velocity. These new parameters strongly prefer the more massive models than previously considered. Now it is also possible that the star could be in the main sequence stage. Using the oscillation spectrum as a gauge, we intend to establish which stage of evolution corresponds better to HD 163899.


2005 ◽  
Vol 40 (9-10) ◽  
pp. 2239-2243 ◽  
Author(s):  
I. Egry
Keyword(s):  

1986 ◽  
Vol 300 ◽  
pp. 773 ◽  
Author(s):  
P. Demarque ◽  
D. B. Guenther ◽  
W. F. van Altena

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