VBLUW-photometry of stars in small fields around 13 planetary nebulae

Details VBLUW-photometry of stars in small fields around 13 planetary nebulae VBLUW-photometry of stars in small fields around 13 planetary nebulae

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...60..399g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 60, June 1985, p. 399-423. Research supported by the Stichti

Astronomy and Astrophysics

Astrophysics

7

Astronomical Maps, Planetary Nebulae, Star Distribution, Stellar Spectrophotometry, Distance

Scientific paper

Observations of stars in small fields around 13 planetary nebulae, made using the Walraven five-channel VBLUW photometer, are presented and described. The fields are found to have a radius of about 0.3 deg. The finding charts for the measured stars are given. It is shown that most stars are brighter than mV of about 14 mag and that the photometry has an accuracy of better than 1 percent, except for stars that are observed with short test-integrations and for stars fainter than mV of about 14 mag. The photometric data for all stars are presented, together with a list of identifications and spectral types.

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