High spectral resolution observations of HD 44179 at 3.2-3.7 microns

Details High spectral resolution observations of HD 44179 at 3.2-3.7 microns High spectral resolution observations of HD 44179 at 3.2-3.7 microns

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...328..709t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 328, May 15, 1988, p. 709-713.

Astronomy and Astrophysics

Astronomy

24

Aromatic Compounds, Far Infrared Radiation, Infrared Spectra, Interstellar Matter, Spectral Resolution, Stellar Coronas, High Resolution, Infrared Astronomy Satellite, Infrared Telescopes

Scientific paper

New high-resolution spectra of HD 44179 (the 'Red rectangle') in the
3.2-3.7 micron range are presented. Contrary to previous observations,
no evidence is found for the 3.4 micron feature which is supposed to
arise from aromatic hydrocarbons. The strong 3.29 micron feature is
found to be different from that seen in NGC 7027 and IRAS 21282+5050.

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