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- W2493014101 abstract "We have obtained a distance of 300 ± 50 pc for the dark cloud L1251 by measuring the colour excess values of 52 field stars around the cloud. In order to find the stars born in L1251, we have combined the information extracted from the IRAS observations with the results of a Schmidt survey for Hα emission stars. Twelve optically visible emission line stars are found within the cloud area. These objects are most probably T Tauri stars. In the same area there are 16 IRAS point sources with fluxes typical of young stellar objects. They form a heterogeneous group containing objects in various evolutionary stages. Five of the Hα emission stars were also detected by IRAS and their pre-main-sequence nature can be considered relatively certain" @default.
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- W2493014101 date "1993-05-01" @default.
- W2493014101 modified "2023-09-24" @default.
- W2493014101 title "Star formation in L 1251 : distance and members." @default.
- W2493014101 hasPublicationYear "1993" @default.
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