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- W1551254356 abstract "An objective-prism survey in the infrared of a region 4°6, square centred on the Pleiades has been made with the Vatican Schmidt and its 2°5 prism in a search for M dwarf members of this cluster. One hundred and twenty-five stars have been classified into four natural groups which correspond to possible dwarfs in the spectral ranges M2-M3, M0-M1, K7-K9 and to non-member field giants of types M0-M4. Provisional blue magnitudes have been obtained by photographic interpolation from photo-electric B magnitudes of Johnson and Mitchell using an electronic reduction programme by Bertiau which incorporates a sky background correction. Positional, photometric, proper motion and spectral data are provided in a catalogue which is supplemented by individual identification charts. An analysis of the surface distribution, magnitudes and proper motions of the stars indicates that the first three groups contain many cluster members. A select list contains 27 stars mostly fainter than B = 16 which are considered probable cluster members. The material is discussed in relation to the evolutionary status of the cluster. Our results show that a well-populated main sequence of early M stars is present down to B = 17." @default.
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- W1551254356 date "1966-01-01" @default.
- W1551254356 modified "2023-09-25" @default.
- W1551254356 title "M stars in the region of the Pleiades" @default.
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- W1551254356 doi "https://doi.org/10.1017/s0074180900053730" @default.
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