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Ultraviolet and optical studies of binaries with luminous cool primaries and hot companions. II - BVRI observations Johnson system BVRI measurements are presented for 117 stars, most ofthem with no previous R and I photometry and many with no previous B andV. The prime objects for measurement are unresolved or nearly unresolvedbinaries containing a late-type giant or supergiant and an early-typecompanion. Other objects on the program include suspected binaries andother F-G giants and supergiants lacking at least R and I magnitudes.The variable F and G supergiants 1 Mon, 89 Her, HR 7308, HR 8157, HR8752, and rho-Cas and the eclipsing systems W Ser and ST Aqr wereobserved; HR 8752 showed significant dimming and cooling over 125 days.Several of Halliwell's (1979) candidates for nearby stars were measured.
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Gözlemler ve gökölçümü verileri
Takýmyýldýz: | Ikizler |
Sað Açýklýk: | 06h20m28.33s |
Yükselim: | +21°32'14.0" |
Görünürdeki Parlaklýk: | 9.646 |
özdevim Sað Açýklýk: | 3.3 |
özdevim Yükselim: | -7.9 |
B-T magnitude: | 9.624 |
V-T magnitude: | 9.645 |
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