Five-colour photometry of blue stars in the Magellanic-Cloud region

Details Five-colour photometry of blue stars in the Magellanic-Cloud region Five-colour photometry of blue stars in the Magellanic-Cloud region

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26as...43..127w&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 43, Jan. 1981, p. 127-140.

Astronomy and Astrophysics

Astrophysics

3

Magellanic Clouds, Stellar Spectrophotometry, Ubv Spectra, Hydrogen Clouds, Tables (Data)

Scientific paper

The results of photoelectric observations of about 500 stars in and between the Magellanic Clouds are given. The observations were made in the Walraven VBLUW-system. Within the limits of the study, no cloud members are found to be associated with the neutral hydrogen between the clouds. Seventy-five stars, previously reported to be cloud members by others, were found independently. A large number of new members of the wing system of the SMC are identified. The great eastward extension of the wing system is clearly illustrated by the results

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