New LRS spectra for 356 bright IRAS sources

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

143

Astronomical Spectroscopy, Infrared Sources (Astronomy), Spaceborne Astronomy, Astronomical Catalogs, Carbon Stars, Continuous Spectra, Cyclic Hydrocarbons, H Ii Regions, Infrared Astronomy Satellite, Silicates, Silicon Carbides, Wolf-Rayet Stars

Scientific paper

The low-resolution spectra of all IRAS point sources with F(nu) (12 microns) greater than 40 Jy that were not included in the Atlas of Low-Resolution Spectra are presented. These have been classified into eight groups based upon the spectral morphology. Silicate emission spectra and red-continuum spectra associated with H II region sources form about 60 percent of this sample. All types of spectra in the LRS Atlas are represented in the sample except for emission-line sources. The sample is used to test a recent classification scheme for IRAS sources based on broadband colors. The spectra is used to test a recent classification scheme for IRAS sources based on broadband colors. The spectra are consistent with the classifications from the colors in most cases.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

New LRS spectra for 356 bright IRAS sources does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with New LRS spectra for 356 bright IRAS sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New LRS spectra for 356 bright IRAS sources will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-761096

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.