UBV surface brightness photometry of the Milky Way in Scorpius from the space probe HELIOS 1

Details UBV surface brightness photometry of the Milky Way in Scorpius from the space probe HELIOS 1 UBV surface brightness photometry of the Milky Way in Scorpius from the space probe HELIOS 1

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....65..245h&link_type=abstract

Astronomy and Astrophysics, vol. 65, no. 2, Apr. 1978, p. 245-249. Research supported by the Alexander von Humboldt-Stiftung; B

Astronomy and Astrophysics

Astronomy

5

Helios 1, Milky Way Galaxy, Stellar Luminosity, Stellar Spectrophotometry, Ubv Spectra, Brightness, Electrophotometers, Satellite Observation, Scorpius Constellation, Spaceborne Astronomy

Scientific paper

Four strips of constant ecliptical latitude in the Milky Way are evaluated for brightness by the zodiacal light experiment on the Helios 1 space probe. Attention is given to UBV data for the Milky Way in Scorpius as reported by the -16 deg photometer. The spectral response is close to the standard UBV system, with effective wavelengths of 364, 427, and 539 nm for a solar type spectrum. Results were compared to previous photometries and predictions from star counts.

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