Near infrared spectroscopy of the supernova remnant RCW103

Details Near infrared spectroscopy of the supernova remnant RCW103 Near infrared spectroscopy of the supernova remnant RCW103

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.290..203o&link_type=abstract

In ESA, Infrared Spectroscopy in Astronomy p 203-205 (SEE N90-19084 11-89)

Astronomy and Astrophysics

Astronomy

1

Infrared Spectroscopy, Line Spectra, Near Infrared Radiation, Supernova Remnants, Deuterium, Hydrogen Ions, Infrared Telescopes, Iron, Spectrum Analysis

Scientific paper

The spectroscopic observations of RCW103 supernova remnants, concerning the Fe II, H2, and hydrogen lines, are reported. The RCW103 is the most powerful source of infrared lines emission among the galactic remnants. The flux calibrated spectrum covering the H and K atmospheric windows, the H2 peak and most of the 1.0 to 1.35 microns wavelength region, are given.

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