Figure 4 from THE MULTIPLICITY OF MASSIVE STARS: A HIGH ANGULAR RESOLUTION SURVEY WITH THE HST FINE GUIDANCE SENSOR

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THE MULTIPLICITY OF MASSIVE STARS: A HIGH ANGULAR RESOLUTION SURVEY WITH THE HST FINE GUIDANCE SENSOR

Authors: E. J. Aldoretta, S. M. Caballero-Nieves, D. R. Gies, E. P. Nelan, D. J. Wallace, W. I. Hartkopf, T. J. Henry, W.-C. Jao, J. Maíz Apellániz, B. D. Mason, A. F. J. Moffat, R. P. Norris, N. D. Richardson, and S. J. Williams

2015 The Astronomical Journal 149 26.

Provider: AAS Journals

Caption: Figure 4.

Histograms of the multiplicity fraction (MF) plotted as a function of orbital period. From top to bottom, successive panels show the distributions for the spectroscopic binary (SB), Fine Guidance Sensor (FGS), Washington Double Star (WDS), and total samples, respectively.

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