Infrared extinction in the Small Magellanic Cloud

Details Infrared extinction in the Small Magellanic Cloud Infrared extinction in the Small Magellanic Cloud

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..895n&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Dec. 15, 1984, p. 895-900.

Astronomy and Astrophysics

Astronomy

9

Astronomical Photometry, Early Stars, Infrared Astronomy, Interstellar Extinction, Magellanic Clouds, Astronomical Models, Galactic Radiation, Stellar Color, Supergiant Stars, Ultraviolet Photometry

Scientific paper

JHK photometry of bright reddened and unreddened early-type SMC members is presented, and the extinction law in those wavebands is studied. VRI photometry of several early-type SMC members is also presented and combined with existing observations to study the extinction at R and I also. It is found that, within the errors, the extinction law from V to K is the same for the SMC as for the Galaxy and the LMC, despite differences previously found in the ultraviolet.

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