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Polarimetric investigation of background stars in the region of T and RY Tau
Electropolarimetric observations of 97 background stars in the TTauri/RY Tauri region, obtained with the 40-cm Cassegrain telescope ofthe Biurakan Astrophysical Observatory in December 1982, are reportedand interpreted in terms of local-magnetic-field effects oncometary-nebula bending. The data are presented in a table, and thedependence of polarization position angle on declination is establishedin a graph and attributed to a continuous variation in the direction ofthe magnetic field. From the magnitude of the effect, however, it isconcluded that the observed bending of the cometary nebulae in theregion results from the combined influence of the local magnetic momentand the magnetic moment of the star itself (as proposed by Vardanian,1983) rather than from the local moment alone.
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| Сазвежђа: | Бик |
| Ректацензија: | 04h24m00.96s |
| Deклинација: | +21°32'26.2" |
| Apparent магнитуда: | 8.806 |
| Proper motion RA: | 9.3 |
| Proper motion Dec: | -8.8 |
| B-T magnitude: | 9.171 |
| V-T magnitude: | 8.837 |
Каталог и designations:
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