scholarly journals Some Uses of Spectral Classification in HR Diagrams

1978 ◽  
Vol 80 ◽  
pp. 3-4
Author(s):  
W.W. Morgan

The MK spectrum-luminosity class diagram (S-LC diagram) between types 09 and G0 is a two-dimensional array containing approximately 100–150 information elements; each information element is a single cell denoted by a spectral type and a luminosity class. These individual, non-dimensional cells (i.e. AO III) can be considered as carriers of observational information toward the HR diagram. Some categories of peculiar spectra (for example, spectra resembling that of the “silicon star” θ Aur) can be attached to certain cells, and can be considered as local perturbations upon the underlying continuity of the spectrum-luminosity class sequences. By such a procedure, the S-LC diagram cells can be considered open-ended, in that progressive additions to the cells can be made indefinitely into the future. Such a procedure can incorporate successfully an unlimited variety of “normal” and “peculiar” categories of spectra - both those already known and those still to be discovered. A morphological system that is unitary thus comes into existence - a system of considerable astrophysical interest. The translation of the detailed language of this system into that of the classical HR diagram is a task for the future.

1979 ◽  
Vol 47 ◽  
pp. 51-58
Author(s):  
Nancy Houk

AbstractA brief review and summary of results from Volumes 1 (-90° to -53°) and 2 (-53° to -40°) of the University of Michigan Catalogue of Two-Dimensional Spectral Types for the HP Stars is given. Plans for the classification of the remaining southern HD stars are outlined. Future plans for observation and classification of northern stars are discussed, including the problem of whether to limit such classification to the HD stars. More general remarks about spectral classification in the future, especially for fainter stars, conclude the paper.


1973 ◽  
Vol 50 ◽  
pp. 258-266
Author(s):  
A. Gutiérrez-Moreno ◽  
H. Moreno

Spectrophotometric data of early type stars (spectral intensity distributions from 3100 to 6000 Å and equivalent widths of Hβ, Hγ and Hδ) have been analysed, looking for the best parameters for a two dimensional spectral classification. It was found that the best correlation with MK classification is given by the equivalent width of Hβ and the Balmer discontinuity.The classification scheme is well defined for stars from B0 to A1 of luminosity classes V to III. No stars of luminosity class II were observed. Luminosity class I is clearly separated from the less luminous stars, but the number of supergiants observed is too small to give a clear separation of spectral types.


1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.


Author(s):  
Chun Zhao ◽  
Tianshi Zhao ◽  
Zongjie Shen ◽  
Yixin Cao ◽  
Yina Liu ◽  
...  
Keyword(s):  

2016 ◽  
Vol 33 (1) ◽  
pp. 119-126 ◽  
Author(s):  
Lucile Gaultier ◽  
Clément Ubelmann ◽  
Lee-Lueng Fu

AbstractConventional altimetry measures a one-dimensional profile of sea surface height (SSH) along the satellite track. Two-dimensional SSH can be reconstructed using mapping techniques; however, the spatial resolution is quite coarse even when data from several altimeters are analyzed. A new satellite mission based on radar interferometry is scheduled to be launched in 2020. This mission, called Surface Water and Ocean Topography (SWOT), will measure SSH at high resolution along a wide swath, thus providing two-dimensional images of the ocean surface topography. This new capability will provide a large amount of data even though they are contaminated with instrument noise and geophysical errors. This paper presents a tool that simulates synthetic observations of SSH from the future SWOT mission using SSH from any ocean general circulation model (OGCM). SWOT-like data have been generated from a high-resolution model and analyzed to investigate the sampling and accuracy characteristics of the future SWOT data. This tool will help explore new ideas and methods for optimizing the retrieval of information from future SWOT missions.


Author(s):  
Dagmar Grimm

Convinced that art should be an expression of life representing the vitality of the times, four architecture students in Dresden joined together to found Die Brücke [The Bridge] in 1905. The name, suggested by one of their founding members, Karl Schmidt-Rottluff, reflected their intention to provide a bridge between the art of previous generations and that of the new era of the twentieth century. As the initiator of Die Brücke and its chief spokesman, Ernst Ludwig Kirchner had the audacious idea of renewing German art. He was joined by Fritz Bleyl, Erich Heckel, and Karl Schmidt-Rottluff, fellow students studying at Dresden’s Technische Hochschule [Dresden Technical Institute]. In preceding years, both Kirchner, who had taken leave of absence to study art, and Bleyl had been working on woodcuts influenced heavily by the earlier Jugendstil. While Bleyl remained interested in the illusion of space, Kirchner had begun to simplify his style to include greater planarity, with jagged lines providing delineation and contour, creating a two-dimensional effect that was already indicative of his signature stylistic innovations of the future.


1965 ◽  
Vol 141 ◽  
pp. 183 ◽  
Author(s):  
W. A. Hiltner ◽  
W. W. Morgan ◽  
J. S. Neff

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