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• W3217029596 endingPage "264" @default.
• W3217029596 startingPage "264" @default.
• W3217029596 abstract "Abstract Binary stars play a vital role in astrophysical research, as a good fraction of stars are in binaries. Binary fraction (BF) is known to change with stellar mass in the Galactic field, but such studies in clusters require binary identification and membership information. Here, we estimate the total and spectral-type high-mass-ratio (HMR) BF ( f 0.6 ) in 23 open clusters using unresolved binaries in color–magnitude diagrams using Gaia DR2 data. We introduce the segregation index ( <?CDATA ${ mathcal S }{ mathcal I }$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mi mathvariant=italic></mml:mi> <mml:mi mathvariant=italic></mml:mi> </mml:math> ) parameter to trace mass segregation of HMR (total and mass) binaries and the reference population. This study finds that in open clusters, (1) HMR BF for the mass range 0.4–3.6 M ⊙ (early M to late B-type stars) has a range of 0.12–0.38 with a peak at 0.12–0.20; (2) older clusters have a relatively higher HMR BF; (3) the mass-ratio distribution is unlikely to be a flat distribution and BF (total) ∼(1.5–2.5) × f 0.6 ; (4) a decreasing BF (total) from late B to K-type stars, in agreement with the Galactic field stars; (5) older clusters show radial segregation of HMR binaries; (6) B-type and A–F type HMR binaries show radial segregation in some young clusters suggesting a primordial origin. This study will constrain the initial conditions and identify the major mechanisms that regulate binary formation in clusters. Primordial segregation of HMR binaries could result from massive clumps spatially segregated in the collapse phase of the molecular cloud." @default.
• W3217029596 created "2021-12-06" @default.
• W3217029596 creator A5018029802 @default.
• W3217029596 creator A5042277361 @default.
• W3217029596 creator A5058417414 @default.
• W3217029596 creator A5082674424 @default.
• W3217029596 date "2021-11-25" @default.
• W3217029596 modified "2023-09-29" @default.
• W3217029596 title "High Mass-Ratio Binary Population in Open Clusters: Segregation of Early Type Binaries and an Increasing Binary Fraction with Mass" @default.
• W3217029596 cites W147232447 @default.
• W3217029596 cites W1966333385 @default.
• W3217029596 cites W1973278676 @default.
• W3217029596 cites W1976100399 @default.
• W3217029596 cites W1979271265 @default.
• W3217029596 cites W1987914079 @default.
• W3217029596 cites W1989522864 @default.
• W3217029596 cites W1997308629 @default.
• W3217029596 cites W1999424690 @default.
• W3217029596 cites W2007958786 @default.
• W3217029596 cites W2011301426 @default.
• W3217029596 cites W2011569645 @default.
• W3217029596 cites W2016888075 @default.
• W3217029596 cites W2031536848 @default.
• W3217029596 cites W2031645757 @default.
• W3217029596 cites W2039737979 @default.
• W3217029596 cites W2045757511 @default.
• W3217029596 cites W2054088499 @default.
• W3217029596 cites W2055745258 @default.
• W3217029596 cites W2056755256 @default.
• W3217029596 cites W2070606946 @default.
• W3217029596 cites W2078262162 @default.
• W3217029596 cites W2080296679 @default.
• W3217029596 cites W2084758952 @default.
• W3217029596 cites W2091327624 @default.
• W3217029596 cites W2093290709 @default.
• W3217029596 cites W2093946497 @default.
• W3217029596 cites W2117673689 @default.
• W3217029596 cites W2123044870 @default.
• W3217029596 cites W2123773590 @default.
• W3217029596 cites W2136742711 @default.
• W3217029596 cites W2140137154 @default.
• W3217029596 cites W2142297733 @default.
• W3217029596 cites W2153646339 @default.
• W3217029596 cites W2213126889 @default.
• W3217029596 cites W2240401013 @default.
• W3217029596 cites W2342249984 @default.
• W3217029596 cites W2752484966 @default.
• W3217029596 cites W2795833838 @default.
• W3217029596 cites W2798336535 @default.
• W3217029596 cites W2888000739 @default.
• W3217029596 cites W2888357359 @default.
• W3217029596 cites W2888469390 @default.
• W3217029596 cites W2908554393 @default.
• W3217029596 cites W2908727800 @default.
• W3217029596 cites W2925297590 @default.
• W3217029596 cites W2973604884 @default.
• W3217029596 cites W2979943038 @default.
• W3217029596 cites W2990988357 @default.
• W3217029596 cites W2991111295 @default.
• W3217029596 cites W3034110725 @default.
• W3217029596 cites W3048964200 @default.
• W3217029596 cites W3098047169 @default.
• W3217029596 cites W3098364059 @default.
• W3217029596 cites W3098624753 @default.
• W3217029596 cites W3098760466 @default.
• W3217029596 cites W3099076641 @default.
• W3217029596 cites W3100463568 @default.
• W3217029596 cites W3100644349 @default.
• W3217029596 cites W3100852845 @default.
• W3217029596 cites W3101131904 @default.
• W3217029596 cites W3102191993 @default.
• W3217029596 cites W3102386126 @default.
• W3217029596 cites W3102467334 @default.
• W3217029596 cites W3103145119 @default.
• W3217029596 cites W3103624749 @default.
• W3217029596 cites W3104373766 @default.
• W3217029596 cites W3105319714 @default.
• W3217029596 cites W3106277786 @default.
• W3217029596 cites W3109131432 @default.
• W3217029596 cites W3110700354 @default.
• W3217029596 cites W3122886126 @default.
• W3217029596 cites W3123154356 @default.
• W3217029596 cites W3124073635 @default.
• W3217029596 cites W3125889973 @default.
• W3217029596 cites W3128624141 @default.
• W3217029596 cites W3134147613 @default.
• W3217029596 cites W3190578944 @default.
• W3217029596 cites W4289710129 @default.
• W3217029596 cites W4292508511 @default.
• W3217029596 cites W4293417884 @default.
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• W3217029596 doi "https://doi.org/10.3847/1538-3881/ac2571" @default.
• W3217029596 hasPublicationYear "2021" @default.
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