Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...74...73f&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 74, no. 1, July 1988, p. 73-81. Sponsorship: Coordenacao do
Astronomy and Astrophysics
Astrophysics
7
A Stars, F Stars, H Beta Line, Interstellar Matter, Stellar Spectrophotometry, Ubv Spectra, Interstellar Extinction, Magellanic Clouds
Scientific paper
As a second part of an investigation of the distribution of interstellar dust in the solar vicinity, uvbyß photometry has been obtained for 260 stars of spectral types A and F, and brighter than mpg = 11m.0 in SA 95, SA 120, SA 168, and SA 200. They are centered at intermediate galactic latitudes, in the range from b ≈ -38° to -42°. SA 95 is almost in the same direction of the Lynds' cloud L1569, and part of it is inside the area's boundaries. Part of the Small Magellanic Cloud has the same line of sight as SA 200. From the observed (b-y) versus β diagrams it can be seen that stars in SA 95 are strongly affected by reddening, while the other areas show very little absorption.
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