Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...237..296s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 237, no. 2, Oct. 1990, p. 296-318.
Astronomy and Astrophysics
Astrophysics
39
Infrared Radiation, Magellanic Clouds, Metallicity, Stellar Evolution, Abundance, Color-Color Diagram, Cosmic Dust, Emission Spectra, Hertzsprung-Russell Diagram
Scientific paper
Infrared Astronomical Satellite (IRAS) maps of the Magellanic Clouds smoothed to a 5-min angular resolution and young star catalogs are used to study the effects of stellar age and metallicity on the infrared emission of these galaxies. The construction of the stellar catalog is described, along with the conversion from the observational to the theoretical temperature-luminosity diagram and the derivation of stellar ages. The infrared color-color diagram of the Clouds is investigated, and the effect of stellar age on their infrared emission is investigated. The effects of the UV radiation field and of the metallicity on the infrared emission are also considered with emphasis on the influence of such parameters as gas-to-dust ratio on the infrared colors. It is shown that the far-infrared fluxes of individual pixels in the Clouds' maps follow the same behavior as the integrated emission of normal galaxies in the IRAS color-color diagram and that the precise position of a particular pixel depends on the age of the youngest star in that pixel.
Sauvage Marc
Thuan Trinh Xuan
Vigroux Laurant
No associations
LandOfFree
The effects of stellar age and metallicity on the infrared emission in the Magellanic Clouds 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 The effects of stellar age and metallicity on the infrared emission in the Magellanic Clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The effects of stellar age and metallicity on the infrared emission in the Magellanic Clouds will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1301164