scholarly journals Line intensities of 12C2H2 in the 7.7μm spectral region

2009 ◽  
Vol 110 (18) ◽  
pp. 2102-2114 ◽  
Author(s):  
L. Gomez ◽  
D. Jacquemart ◽  
N. Lacome ◽  
J.-Y. Mandin
Keyword(s):  
Spectral Region ◽  
Line Intensities

Line intensities in the 1.5-μm spectral region of acetylene

2007 ◽  
Vol 108 (3) ◽  
pp. 342-362 ◽  
Author(s):  
H. Tran ◽  
J.-Y. Mandin ◽  
V. Dana ◽  
L. Régalia-Jarlot ◽  
X. Thomas ◽  
...  
Keyword(s):  
Spectral Region ◽  
Line Intensities

Absolute line intensities for oxirane in the 11.4 μm spectral region

2013 ◽  
Vol 112 (12) ◽  
pp. 1633-1638 ◽  
Author(s):  
F. Kwabia Tchana ◽  
J.-M. Flaud ◽  
W.J. Lafferty ◽  
M. Ngom
Keyword(s):  
Spectral Region ◽  
Line Intensities

Line intensities of acetylene: New measurements in the 1.5-μm spectral region and global modelling in the ΔP=10 series

2009 ◽  
Vol 110 (17) ◽  
pp. 1815-1824 ◽  
Author(s):  
O.M. Lyulin ◽  
V.I. Perevalov ◽  
H. Tran ◽  
J.-Y. Mandin ◽  
V. Dana ◽  
...  
Keyword(s):  
Spectral Region ◽  
Line Intensities ◽  
Global Modelling

Line intensities of acetylene: Measurements in the 2.5-μm spectral region and global modeling in the and 6 series

2007 ◽  
Vol 103 (3) ◽  
pp. 496-523 ◽  
Author(s):  
O.M. Lyulin ◽  
V.I. Perevalov ◽  
J.-Y. Mandin ◽  
V. Dana ◽  
F. Gueye ◽  
...  
Keyword(s):  
Spectral Region ◽  
Global Modeling ◽  
Line Intensities

12C16O2 line intensities in the 4.8 μm spectral region

1994 ◽  
Vol 52 (3-4) ◽  
pp. 333-340 ◽  
Author(s):  
V. Dana ◽  
J.-Y. Mandin ◽  
A. Barbe ◽  
J.-J. Plateaux ◽  
L.S. Rothman ◽  
...  
Keyword(s):  
Spectral Region ◽  
Line Intensities

Line Intensities of 12C16O2 in the 1.2–1.4 μm Spectral Region

2000 ◽  
Vol 201 (2) ◽  
pp. 249-255 ◽  
Author(s):  
J.-L. Teffo ◽  
C. Claveau ◽  
Q. Kou ◽  
G. Guelachvili ◽  
A. Ubelmann ◽  
...  
Keyword(s):  
Spectral Region ◽  
Line Intensities

scholarly journals Two Possible Wind Models for Wolf-Rayet stars

1986 ◽  
Vol 116 ◽  
pp. 223-224
Author(s):  
T. Nugis
Keyword(s):  
Emission Line ◽  
Observational Data ◽  
Spectral Region ◽  
Constant Velocity ◽  
Empirical Models ◽  
The Other ◽  
Spherically Symmetric ◽  
Line Intensities ◽  
Velocity Zone ◽  
The Continuum

Frequently the models proposed to explain some observational data are in conflict with the other observational data. Our purpose was to find out the empirical models of the envelopes of WN5 and WN6 stars which are not in conflict with the continuum runs in the IR spectral region and with the emission line intensities and profiles. In our recent study (Nugis, 1984) we proposed for Wolf-Rayet stars the spherically symmetric outflow model having an increasing velocity zone (with some coronal heating near the stellar surface) which is followed by the decreasing velocity zone extending up to the distance where the matter starts flowing with constant velocity. Let us call this model the AD-model (Acceleration-Deceleration).

Line intensities of hot bands in the spectral region of acetylene 12C2H2

2001 ◽  
Vol 69 (1) ◽  
pp. 81-101 ◽  
Author(s):  
D. Jacquemart ◽  
C. Claveau ◽  
J.-Y. Mandin ◽  
V. Dana
Keyword(s):  
Spectral Region ◽  
Line Intensities

On the Inhomogeneity of Chemical Composition over the Surface of 21 Per

1976 ◽  
Vol 32 ◽  
pp. 343-349
Author(s):  
Yu.V. Glagolevsky ◽  
K.I. Kozlova ◽  
V.S. Lebedev ◽  
N.S. Polosukhina
Keyword(s):  
Chemical Composition ◽  
Spectral Line ◽  
Variable Star ◽  
Radial Velocities ◽  
Crimean Astrophysical Observatory ◽  
Line Intensities ◽  
Magnetic Variable

SummaryThe magnetic variable star 21 Per has been studied from 4 and 8 Å/mm spectra obtained with the 2.6 - meter reflector of the Crimean Astrophysical Observatory. Spectral line intensities (Wλ) and radial velocities (Vr) have been measured.

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