Reddening relations of the VBLUW and UBV systems for objects with emission line spectra

Details Reddening relations of the VBLUW and UBV systems for objects with emission line spectra Reddening relations of the VBLUW and UBV systems for objects with emission line spectra

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...111..185d&link_type=abstract

Astronomy and Astrophysics, vol. 111, no. 1, July 1982, p. 185-192.

Astronomy and Astrophysics

Astrophysics

4

Emission Spectra, Interstellar Extinction, Line Spectra, Planetary Nebulae, Supernova Remnants, Ubv Spectra, Astronomical Photometry, Black Body Radiation, Hydrogen Clouds, Stellar Spectra

Scientific paper

For the Walraven VBLUW and Johnson UBV system, reddening relations are investigated for emission line objects: emission nebulae, planetary nebulae, supernova remnants. In contrast with the reddening relations derived empirically for supernova remnants, the reddening relations calculated for planetary nebulae and emission nebulae seem to be different from the known reddening relations derived for stars, i.e. continuum sources.

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