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GasDust Shells around Some Early-Type Stars with an IR Excess (of Emission)
The results of an investigation of IR (IRAS) observations of 58OBAF stars of different luminosity classes, whichare mainly members of various associations, are presented. The colorindices of these stars are determined and two-color diagrams areconstructed. The emission excesses at 12 and 25 mm (E 12 and E 25) arealso compared with the absorption A1640 of UV radiation. It is concludedthat 24 stars (of the 58 investigated) are disk systems of the Vegatype, to which Vega = N 53 also belongs. Eight known stars of the Vegatype are also given in the figures for comparison. The remaining 34stars may have gasdust shells and/or shelldisks. The IRemission excesses of the 34 investigated stars and 11 comparison stars(eight of them are Be-Ae stars) are evidently due both to thermalemission from grains and to the emission from freefreetransitions of electrons in the gasdust shells of these stars.
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| Takýmyýldýz: | Tukan |
| Sað Açýklýk: | 00h24m46.37s |
| Yükselim: | -58°00'51.3" |
| Görünürdeki Parlaklýk: | 9.384 |
| özdevim Sað Açýklýk: | 50.8 |
| özdevim Yükselim: | 4.6 |
| B-T magnitude: | 9.776 |
| V-T magnitude: | 9.417 |
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