Infrared (FeII), H and H2 lines in galaxy nuclei

Details Infrared (FeII), H and H2 lines in galaxy nuclei Infrared (FeII), H and H2 lines in galaxy nuclei

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.290..507m&link_type=abstract

In ESA, Infrared Spectroscopy in Astronomy p 507-509 (SEE N90-19084 11-89)

Astronomy and Astrophysics

Astronomy

3

Galactic Nuclei, H Ii Regions, Hydrogen Recombinations, Infrared Spectroscopy, Iron, Line Spectra, Hydrogen Clouds, Hydrogen Ions, Infrared Spectra, Molecular Clouds, Seyfert Galaxies

Scientific paper

The preliminary results of the spectroscopic of Fe II, H2 and hydrogen recombination line emission are presented. Selected galaxies from a sample of 35, ranging from pure H II region-like to Seyfert 1, are studied. The studies were carried out with the infrared spectrometer IRSPEC at the European Southern Observatory (Chile) 3.6 m telescope. The observations include measurements of additional lines of diagnostic interest: the H2(2 1S(1)) line at 2.247 microns improved linewidth determinations and some limited spatial mapping.

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