Lutheran Ladies’ Seminary at Red Wing, Minnesota

Unstoppable ◽  
2020 ◽  
pp. 264-319
Keyword(s):  
Red Wing

Red-Wing

1986 ◽  
Vol 11 (1) ◽  
pp. 8-9
Author(s):  
Larry J. Zimmerman
Keyword(s):  
Red Wing

scholarly journals Collisional effects in the far red wing of Lyman-$\sf \alpha$

2008 ◽  
Vol 493 (3) ◽  
pp. 1155-1160 ◽  
Author(s):  
N. F. Allard ◽  
J. F. Kielkopf
Keyword(s):  
Red Wing

scholarly journals Slow and Rapid Changes of the Radial Velocities in the Symbiotic Binary CH Cygni

1988 ◽  
Vol 103 ◽  
pp. 223-224
Author(s):  
A. Skopal
Keyword(s):  
Light Curve ◽  
Orbital Motion ◽  
Radial Velocities ◽  
Cool Component ◽  
Absorption Component ◽  
Middle Position ◽  
Rapid Changes ◽  
Red Wing

In the period 1982–1986, new 98 radial velocities (RVs) were determined (at the figures denoted by □). All spectrograms were obtained at the Toruń Observatory. RVs were measured at the Skalnaté Pleso Observatory. The main results are summarized in the figures 1-3. The phase is determined from the middle position of the hot component eclipse (JD 2 446 272) and from the minima difference observed in U light curve (5700d) (Mikolajewski et al., 1987).Slow changes of the RVs of the absorption components of ionized metals reflect the orbital motion of the hot component only between the phases 0.7 and 0.0. The rapid changes are observed mainly between the phases 0.8 and 0.9. They are created by combination of the emission red wing with the absorption component (Skopal et al., 1987). RVs of the cool component are in antiphase (Tomov and Luud, 1984).

Effects of interaction Hg-C60 observed on the far red wing of the Hg 253.7 nm line

1995 ◽  
Author(s):  
T. Grycuk ◽  
M. Tchaplyguine ◽  
E. Czerwosz ◽  
P. Byszewski
Keyword(s):  
Red Wing

Die Druckverbreiterung der diffusen Heliumlinien, Vergleich zwischen Messung und Theorie im quasistatischen Bereich

1966 ◽  
Vol 21 (6) ◽  
pp. 697-718 ◽  
Author(s):  
H. Pfennig ◽  
E. Trefftz
Keyword(s):  
Stark Effect ◽  
Point Of View ◽  
Spectral Lines ◽  
Experimental Point ◽  
Line Profiles ◽  
Experimental Conditions ◽  
Part D ◽  
Upper Level ◽  
Good Agreement ◽  
Red Wing

It is difficult to discriminate between theories of pressure broadening of spectral lines through comparison with experiments. Line profiles are insensitive with respect to details of the theory, and it is difficult to keep experimental conditions clear and certain enough to make the comparison relevant. We used measurements of VIDAL 1 which are satisfactory from the experimental point of view. The wings of the diffuse He-lines 2P — nD are compared with those calculated by quasistatic theory. Part B deals with STARK effect splitting of the upper level. Part C describes the quasistatic theory of the line wings, and discusses the probability function of the so called micro field strength. In part D the results of the calculation are compared with the measurements. The comparison is relevant only for the violet wings of the triplet series. The red wing of the triplet lines and the violet wing of the singlet lines are disturbed by the forbidden component 2P — nP. The red wing of singlet lines is experimentally too inexact because of disturbing wings of neighboring triplet lines. The slope of the violet side of the triplet wings shows good agreement between theory and measurement for the far wing (large Δv). For decreasing Δv the experimental curve stays below the theoretical curve. For comparison of wing intensities it proves to be important to normalize the line profiles. It is seen that the measured height of the wings increases less with increasing main quantum number than the theoretical height.

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