New Wavelength Determinations of Mid‐Infrared Fine‐structure Lines byInfrared Space ObservatoryShort Wavelength Spectrometer

1997 ◽  
Vol 487 (2) ◽  
pp. 962-966 ◽  
Author(s):  
H. Feuchtgruber ◽  
D. Lutz ◽  
D. A. Beintema ◽  
E. A. Valentijn ◽  
O. H. Bauer ◽  
...  
2002 ◽  
Vol 575 (1) ◽  
pp. 585-586
Author(s):  
Uriel Giveon ◽  
Amiel Sternberg ◽  
Dieter Lutz ◽  
Helmut Feuchtgruber ◽  
A. W. A. Pauldrach

2002 ◽  
Vol 566 (2) ◽  
pp. 880-897 ◽  
Author(s):  
Uriel Giveon ◽  
Amiel Sternberg ◽  
Dieter Lutz ◽  
Helmut Feuchtgruber ◽  
A. W. A. Pauldrach

1997 ◽  
Vol 159 ◽  
pp. 333-336
Author(s):  
D. Lutz ◽  
R. Genzel ◽  
E. Sturm ◽  
A.F.M. Moorwood ◽  
E. Oliva ◽  
...  

AbstractWe discuss 2.5–45 µm spectra of the Circinus galaxy and of Cen A, obtained with the Short Wavelength Spectrometer (SWS) on board the Infrared Space Observatory. The large number of detected ionic fine structure lines, observable also in visually obscured sources, provides strong constraints on the shape of the ionizing spectrum, which is found to exhibit a UV bump peaking at ~ 70 eV in the case of Circinus. Pure rotational emission of molecular hydrogen, directly probing warm molecular gas, can for the first time be detected in external galaxies.


Model theoretical calculations have been made of the fine structure associated with the perpendicular vibrations of a ‘light’ symmetric top group (such as CH 3 , SiH 3 , etc.) resulting from its internal rotation with respect to an infinitely heavy planar framework. Investigations have been made of the effects on the internal rotational fine structure of the removal of the degeneracy of the perpendicular vibrations as required by the lower site symmetry. Separate calculations have been made for the cases where the removal of degeneracy is caused ( a ) by electronic effects which result in an angular variation of the appropriate force constant, or ( b ) by interaction with another vibration in the framework part of the molecule. It is found that no fine structure lines occur between the non-degenerate frequencies, but that the effect of internal rotation is to generate rotational wings outside this frequency range. The effects of a finite sixfold barrier to internal rotation on the vibrational/internal-rotational absorption band have been calculated for the degenerate and non-degenerate cases. It is shown that certain lines are split by amounts comparable to the barrier height, V 6 , which should therefore be experimentally obtainable from this type of spectrum in favourable cases. The effect of an increasing barrier is to cause more of the intensity within the overall band contour to occur in the vicinity of the vibrational frequency or frequencies, and less in the internal rotational wings, as expected on physical grounds.


Author(s):  
D. A. Naylor ◽  
R. Emery ◽  
B. Fitton ◽  
I. Furniss ◽  
R. E. Jennings ◽  
...  

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