Radio Emission from Chemically Peculiar Stars
Abstract
In five VLA observing runs the initial survey of radio emission from magnetic Bp-Ap stars by Drake et al. is extended to include a total of 16 sources detected at 6 cm out of 61 observed, giving a detection rate of 26 percent. Of these stars, three are also detected at 2 cm, four at 3.6 cm, and five at 20 cm. The 11 new stars detected as radio sources have spectral types B5-A0 and are He-weak and Si-strong. No classical (SrCrEu-type) Ap stars have yet been detected. The 16 detected sources show a wide range of radio luminosities with the early-B He-S stars on average 20 times more radio luminous than the late-B He-W stars and 1000 times more luminous than Theta Aurigae. Multifrequency observations indicate flat spectra in all cases. Four stars have a detectable degree of circular polarization at one or more frequencies. It is argued that the radio-emitting CP (chemically peculiar) stars form a distinct class of radio stars that differs from both the hot star wind sources and the active late-type stars. The observed properties of radio emission from these stars may be understood in terms of optically thick gyrosynchrotron emission from a nonthermal distribution of electrons produced in a current sheet far from the star. In this model the electrons travel along magnetic fields to smaller radii and higher magnetic latitudes where they mirror and radiate microwave radiation.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- July 1992
- DOI:
- 10.1086/171509
- Bibcode:
- 1992ApJ...393..341L
- Keywords:
-
- Peculiar Stars;
- Radio Emission;
- Radio Sources (Astronomy);
- Stellar Luminosity;
- Very Large Array (Vla);
- Circular Polarization;
- Early Stars;
- Late Stars;
- Stellar Temperature;
- Stellar Winds;
- Astrophysics;
- RADIO CONTINUUM: STARS;
- STARS: CHEMICALLY PECULIAR