Nonthermal radio emission from HD 193793 and V410 Tauri

Details Nonthermal radio emission from HD 193793 and V410 Tauri Nonthermal radio emission from HD 193793 and V410 Tauri

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...297..649b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 297, Oct. 15, 1985, p. 649-651.

Astronomy and Astrophysics

Astrophysics

44

Emission Spectra, Nonthermal Radiation, Pre-Main Sequence Stars, Radio Emission, Stellar Spectrophotometry, Variable Stars, Wolf-Rayet Stars, Centimeter Waves, Spectral Resolution, Stellar Evolution, Thermal Emission

Scientific paper

Radio observations of the Wolf-Rayet star HD 193793 and the
pre-main-sequence star V410 Tau lead to the conclusion that both stars
are sources of nonthermal radio emission. In particular, the emission
from HD 193793 is unresolvable by the VLA, while the emission from V410
Tau is highly variable.

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