ζ Orionis A is a Double Star

By C. Hummel, N. White, N. M. Elias, A. Hajian, T. Nordgren. 2000

206 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/ccfcfc5a0b15b4ba6b34844c72d366e0d0c8493e

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In Astronomy and Astrophysics

1. B. Mason
2. W. Hartkopf
3. D. Gies
4. A. Tokovinin
5. N. Turner
6. T. Henry
7. T. T. ten Brummelaar
8. Lewis C. Roberts Jr.

Citations in the corpus

• Dynamical mass of the O-type supergiant in ζ Orionis A (2013, methodology): “Hummel et al. (2000) found a companion 40 mas from the O9.”
• Adaptive Optics Photometry and Astrometry of Binary Stars. II. A Multiplicity Survey of B Stars (2005, background): “Some of the scatter in the residuals may be due to the presence of a closer companion to ζ Ori A found by interferometry (Hummel et al. 2000).”
• THE HIGH ANGULAR RESOLUTION MULTIPLICITY OF MASSIVE STARS (2008, methodology): “These sources were supplemented by detailed studies of specific stars or clusters, such as ζ Ori (long baseline optical interferometry; Hummel et al. 2000), Trumpler 14 (HST FGS; Nelan et al. 2004), the Orion Trapezium (infrared single aperture interferometry; Petr et al. 1998; Simon et al. 1999;…”