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Breger, M · 1993 · DOI 10.1051/0004-6361:1993271482

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astro-ph.SR 1

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2026 1

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The Double-lined Eclipsing $\gamma$ Doradus System AX Draconis in a 0.568-day Orbit

astro-ph.SR · 2026-06-04 · unverdicted · novelty 6.0

AX Dra is characterized as a 0.568-day semi-detached eclipsing binary with component masses 1.717 and 0.804 solar masses, radii 1.541 and 1.237 solar radii, and four independent gamma Dor pulsation frequencies in the primary, making it the shortest such system and suggesting the primary is an accret

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  • The Double-lined Eclipsing $\gamma$ Doradus System AX Draconis in a 0.568-day Orbit astro-ph.SR · 2026-06-04 · unverdicted · none · ref 6

    AX Dra is characterized as a 0.568-day semi-detached eclipsing binary with component masses 1.717 and 0.804 solar masses, radii 1.541 and 1.237 solar radii, and four independent gamma Dor pulsation frequencies in the primary, making it the shortest such system and suggesting the primary is an accret