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- W1626585820 abstract "Trapezia systems are defined as multiple stars, having three or more components with separation ratios in the range 0.3 to 3. The revival of interest in Trapezia is due to their potential astrophysical significance, as they could originate from a single protostar and be in an expansion stage because of their possible positive energy (see, for example, Bernacca 1988 and references therein). Further decisive advancements in understanding the nature of these systems require data for establishing a list of physically bound systems as well as for the systematic study of their kinematics and energetics. In the present progress report we test three representative cases with the combined exploitation of astrometric, photometric, and spectroscopic data." @default.
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- W1626585820 date "1992-01-01" @default.
- W1626585820 modified "2023-09-24" @default.
- W1626585820 title "Astrometry and Photometry of Trapezium–Type Multiple Stars" @default.
- W1626585820 cites W1972092979 @default.
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- W1626585820 doi "https://doi.org/10.1017/s0252921100006618" @default.
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