Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...297..261s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 297, no. 1, p. 261-271
Astronomy and Astrophysics
Astrophysics
8
Distance, Interstellar Extinction, Planetary Nebulae, Stellar Color, Stellar Magnitude, Stellar Radiation, Color-Color Diagram, Line Of Sight, Stellar Spectrophotometry
Scientific paper
Published photoelectric UBV photometry of stars in the angular vicinity (radius = 15') of three planetary nebulae was used to construct a reddening distance relation for the line of sight towards each planetary nebula. This relation was confirmed by data on nearby stars and star clusters from the literature. The distances derived are 800 +/- 300 pc for PN G128.0-04.1 (S 188, Simeiz 22), 800 +/- 400 pc for PN G149.4-09.2 (HDW 3), and 1100 +/- 300 pc for PN G224.9+01.0 (We 1-6).
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