Revised spectrographic and photometric elements of ZZ Boo.
Bruno Cester, G. Giuricin, Fabio Mardirossian, M. Mezzetti
Abstract
Bruno Cester, G. Giuricin, Fabio Mardirossian, M. Mezzetti
Abstract
Some inconsistencies between spectrographic and photoelectric elements of the double-spectrum eclipsing binary ZZ Boo revealed that a set of spectrographic observations should be interchanged. With the newly deduced elements the star appears to be a normal detached system on the upper border of the main sequence. Both components agree well with an isochrone of age 1 billion yr and chemical composition Y = 0.30, Z = 0.004.
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Some inconsistencies between spectrographic and photoelectric elements of the double-spectrum eclipsing binary ZZ Boo revealed that a set of spectrographic observations should be interchanged. With the newly deduced elements the star appears to be a normal detached system on the upper border of the main sequence. Both components agree well with an isochrone of age 1 billion yr and chemical composition Y = 0.30, Z = 0.004.
Key concepts: Photometry (optics), Computer science, Physics, Astrophysics, Stars