Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aj....125..858j&link_type=abstract
The Astronomical Journal, Volume 125, Issue 2, pp. 858-867.
Astronomy and Astrophysics
Astronomy
22
Stars: Binaries: General, Radio Continuum
Scientific paper
Centimeter-wavelength radio observations of the T Tauri system between 1983 and 2001 confirm that the radio emission from the optical star T Tau (T Tau N) has a spectral index of 0.6 and may be attributed to a stellar wind and nonthermal flares that are masked by the thermal emission. Right-circular polarization of 26% is detected in the 2 cm T Tau N emission. The infrared source (T Tau S) is confirmed to be nonthermal and variable in intensity, with a radio spectral index <=0. T Tau S displays weak extended emission and strong, compact left-circular polarization at wavelengths of 3.7 and 2 cm; the percentage of left-circularly polarized emission is larger at the shorter wavelengths. The 2 cm radio and optical positions of T Tau N are found to be coincident to 13 mas. Relative motion between the two radio sources (T Tau N and S) does not agree in detail with that measured at a wavelength of ~2 μm. The difference in relative position is as large as 100 mas (15 AU) in declination in the 1980s. The recent IR detection of T Tau S as a binary star with a separation of 50 mas (7 AU) in 1997 December may explain this discrepancy. We suggest a scenario in which the radio emission detected toward T Tau S in our most recent observations (epoch 2001) is located at the position of the less luminous member of this binary system, T Tau Sb. A preliminary estimate of the orbital parameters of this system is an eccentricity of 0.7, semimajor axis 113 mas, inclination 69°, period 38.8 yr, and total system mass 5.3 Msolar. The circular polarization of the centimeter radio emission of T Tau N and T Tau S indicates that the emission from both components is gyrosynchrotron in nature. The opposite sense of circular polarization may indicate that it is dipole in nature.
Claussen Mark J.
de Vegt Ch.
Fey Alan Lee
Gaume Ralph A.
Johnston Ken J.
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