Four-point optical energy distributions for faint BL Lacertae objects

Details Four-point optical energy distributions for faint BL Lacertae objects Four-point optical energy distributions for faint BL Lacertae objects

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...203..291t&link_type=abstract

Astrophysical Journal, vol. 203, Jan. 15, 1976, pt. 1, p. 291-296. Research supported by AURA, Inc.

Astronomy and Astrophysics

Astronomy

55

Astronomical Photometry, Astronomical Spectroscopy, Quasars, Radiant Flux Density, Radio Sources (Astronomy), Spectral Energy Distribution, Ubv Spectra, Line Shape, Luminous Intensity, Monochromatic Radiation, Spectrophotometry, Spectrum Analysis, Tables (Data)

Scientific paper

Broad-band photoelectric observations of 10 radio sources with continuous optical spectra have been reduced to monochromatic flux densities in order to study the shape and variations of their optical energy distributions. The observed spectral indices range between 1 and 3. It is suggested that sources with a large optical spectral index may have detectable nebulosity.

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