ISO LWS-SWS Observation of IRAS 19120+1103

Details ISO LWS-SWS Observation of IRAS 19120+1103 ISO LWS-SWS Observation of IRAS 19120+1103

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456..215l&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Computer Science

Iso, Stars:Individual:Iras 19120+1103, Ism:Lines And Bands, Infrared:Continuum, Infrared:Stars

Scientific paper

We present observations of the source IRAS 19120+11- 03 taken with both Short and Long Wavelength Spectrometers (SWS, LWS) on board of the Infrared Space Observatory (ISO) satellite. The heated dust enshrouding the central star emits with a Spectral Energy Distribution that is characterized by the peak position at about 100 μm. Here we present original and high quality data of this source. These give a more complete view of this source, since many atomic lines in different ionization state are measured for the first time and many features usually referred to as UIRs (Unidentified Infrared Bands) are detected between 2-200 μm.

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