On interstellar reddening law in the Taurus dark clouds

Details On interstellar reddening law in the Taurus dark clouds On interstellar reddening law in the Taurus dark clouds

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..85..271s&link_type=abstract

Astrophysics and Space Science, vol. 85, no. 1-2, July 1982, p. 271-275.

Astronomy and Astrophysics

Astronomy

25

Interstellar Extinction, Interstellar Matter, Molecular Clouds, Stellar Color, Stellar Spectrophotometry, Ultraviolet Astronomy, Astronomical Photometry, Electrophotometry, Iue, Taurus Constellation

Scientific paper

The interstellar reddening law in the Taurus dark clouds is investigated from visual, infrared, and ground based ultraviolet photometric observations of heavily reddened stars HD 29647, HDE 283701, and HDE 283812. The star HD 29647 located in the center of a very dense dark cloud Khavtassi 278 shows a reddening law which is anomalous in the wavelengths shorter than 400 nm. When combined with observations by Snow and Seab (1980) from the IUE it can be represented by a single straight line from 1 micron to 250 nm. The two other stars situated in less dense parts of the Taurus dark clouds show normal reddening law.

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