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Revised spectrographic and photometric elements of ZZ Boo.

Bruno Cester, G. Giuricin, Fabio Mardirossian, M. Mezzetti

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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.

About this research paper

What this paper is about

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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Available 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.

Key concepts: Photometry (optics), Computer science, Physics, Astrophysics, Stars

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Revised spectrographic and photometric elements of ZZ Boo. — Research Paper | ScholarLens