Anaerobiosis and a Theory of Growth Line Formation

Science ◽  
1977 ◽  
Vol 198 (4323) ◽  
pp. 1222-1227 ◽  
Author(s):  
R. A. Lutz ◽  
D. C. Rhoads
Keyword(s):  
Author(s):  
Margaret R. Deith

The shells of marine invertebrates grow incrementally (Wilbur, 1972). When a section of shell is observed under the microscope, the increments are often visible, separated by fine lines (Fig. 1). Studies of these phenomena have focused chiefly on the periodicity of increment and growth-line formation, principally because of its geological or archaeological application as a ‘biological clock’ (e.g. Wells, 1963; Koike, 1973).


1984 ◽  
Vol 62 (12) ◽  
pp. 2495-2504 ◽  
Author(s):  
Margaret E. Day

Growth records retained in the shell of Lampsilis radiata radiata and shell ultrastructure were examined in a population from Lake Champlain, Vermont, U.S.A. Maximum size was 75 mm as measured from the umbo to the farthest margin. Ages were obtained by counting annual bands, and growth plots were constructed. By knowing the amount grown by individuals of the same age in the same year, the years 1975 and 1977 were identified as poor for growth of younger individuals. Light micrographs of shell thin sections showed macroscopic annual lines, and microscopic and ultrastructural lines. Ultrastructural lines were visible within macroscopic lines. Scanning electron micrographs of etched sections clarified the light micrographs and allowed recognition of two damage-response structures embedded within the nacreous layer in the umbonal region: adventitious conchiolin and prismatic crystals. Theories of growth line formation are presented. Shell growth appears to follow an alternating cycle of protein deposition as organic matrices followed by CaCO3 secretion into the matrices. The Lutz–Rhoads theory of growth line formation, based on alternating periods of aerobic and anaerobic metabolism, was examined in detail and found unsuitable for this species.


2020 ◽  
Vol 237 (2) ◽  
pp. 367-378 ◽  
Author(s):  
Amanda M. Papakyrikos ◽  
Manish Arora ◽  
Christine Austin ◽  
Julia C. Boughner ◽  
Terence D. Capellini ◽  
...  

1973 ◽  
Vol 54 ◽  
pp. 173-221
Author(s):  
J. C. Pecker

Regardless of the degree of elaboration of series of models, just how can they be used for calibration purposes? And how much is this calibration sensitive to the quality of the model theory? These two questions are the basis of our discussion, which covers : I – The general principles of the use of model atmospheres in stellar calibration (1 – The two dimensional classifications; 2 – The use of the total luminosity; 3 – The cases of Vega and Sirius; 4 – The calibration of ST – Teff relation); II – The failures of the two parameters model atmospheres (1 – The observational need for more-than-two-parameters classification; 2 – The abundance of elements, the line formation, and the model atmospheres; 3 – Various sources of unadequacy of models; 4 – Envelopes or shell features; their influence on model-building; 5 – The case of HD 45677. Diagnostic of early-type stars; 6 – Various unexplained spectral features); III – The present state of the model factory (1 – The classical models; 2 – New concepts in the description of a stellar atmosphere; 3 – New approaches in model making; 4 – Conclusions).


2009 ◽  
Vol 500 (3) ◽  
pp. 1221-1238 ◽  
Author(s):  
D. Fabbian ◽  
M. Asplund ◽  
P. S. Barklem ◽  
M. Carlsson ◽  
D. Kiselman

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