Interstellar extinction curve - The profile of very broad structure

Details Interstellar extinction curve - The profile of very broad structure Interstellar extinction curve - The profile of very broad structure

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...166..271k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 166, no. 1-2, Sept. 1986, p. 271-275.

Astronomy and Astrophysics

Astrophysics

15

Interstellar Extinction, Stellar Spectra, Dwarf Stars, Stellar Color, Supergiant Stars, Visible Spectrum

Scientific paper

The interstellar extinction curve between 3500 and 10500 Å is determined from a series of two-colour plots based on existing spectral scans. Very broad structure (VBS) covers the wavelength range from 5000 to 8000 Å and consists of 3 components centered at 5300, 5900 and 6800 Å. The VBS is shown to originate in the same agent as that of continuous extinction.

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