The B and V magnitudes of the central stars of planetary nebulae

Details The B and V magnitudes of the central stars of planetary nebulae The B and V magnitudes of the central stars of planetary nebulae

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...89...77t&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 89, no. 1, July 1991, p. 77-90.

Astronomy and Astrophysics

Astrophysics

60

Early Stars, Planetary Nebulae, Spectrophotometry, Stellar Magnitude, Continuous Spectra, Stellar Spectra

Scientific paper

The B and V magnitudes are determined for about 350 central stars of
planetary nebulae, 190 of which are being given for the first time. The
stellar continuum was measured on spectra taken at ESO, Chile, and at
OHP, France, in range of 400-740 nm, with a resolution of about 1 nm.

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