A photoelectric UBV sequence in a low extinction Puppis field

Details A photoelectric UBV sequence in a low extinction Puppis field A photoelectric UBV sequence in a low extinction Puppis field

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...49..521r&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 49, Aug. 1982, p. 521-527. Research supported by the University of Waterloo.

Astronomy and Astrophysics

Astrophysics

2

Electrophotometry, Interstellar Extinction, Milky Way Galaxy, Stellar Spectra, Ubv Spectra, Early Stars, Galactic Structure, Space Density, Stellar Color, Stellar Luminosity, Stellar Magnitude

Scientific paper

UBV photoelectric photometry, MK-dispersion slit spectra, and spectral classifications based on objective prism spectra are presented for a sequence of 116 early type stars in the Puppis region. The interstellar extinction, based largely on spectroscopic parallaxes, is found to be remarkably low for a field in the Galactic Plane, amounting to 0.30 m for E(B-V) at r of about 6.3 kpc.

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