期刊
ASTRONOMY & ASTROPHYSICS
卷 372, 期 2, 页码 644-650出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20010496
关键词
interstellar medium : dust, extinction
We present new measurements of the interstellar reddening parameter R-V = A(V)/E(B-V) towards 35 O stars. The results are combined with measurements from the literature for 60 stars to study the behaviour of R-V with heliocentric distance. R-V is the single basic parameter which characterizes the interstellar extinction from the near-infrared to the far-UV spectral region. The absolute extinction A(V), from which R-V is derived, is best determined by optical and near-infrared photometry (Cardelli et al. 1989). We consider important the derivation of R-V with the same technique in the direction of as many as possible galactic O stars.
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