Ultraviolet studies of the Magellanic Clouds. I - Observations

Details Ultraviolet studies of the Magellanic Clouds. I - Observations Ultraviolet studies of the Magellanic Clouds. I - Observations

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....86..299m&link_type=abstract

Astronomy and Astrophysics, vol. 86, no. 3, June 1980, p. 299-303.

Astronomy and Astrophysics

Astronomy

14

Magellanic Clouds, Satellite Observation, Ultraviolet Astronomy, Brightness, D-2 Satellites, Ultraviolet Spectra

Scientific paper

Observations with the D2B-Aura satellite are used to derive absolute UV brightness maps of the Magellanic Clouds at 3100, 2200, and 1690 A, with an equivalent resolution of about 3 x 3 deg. Integrated fluxes of the Clouds are calculated and compared with other determinations. Both Clouds have smooth UV spectra, the Small Cloud being bluer than the Large Cloud.

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