Hundreds of stars have now been detected at radio wavelengths. At least four processes are believed to cause the radio emission: thermal bremsstrahlung, gyrosynchrotron, cyclotron maser, and plasma radiation. Here the characteristics of the various classes of detected stars are reviewed, along with the putative reasons for the radio emission. The classes of stars described include: single stars, binaries containing two main sequences and/or giant stars, binaries containing one white dwarf, and binaries containing one neutron star or black hole.


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    Titel :

    Stellar activity at radio wavelengths


    Beteiligte:

    Erschienen in:

    Erscheinungsdatum :

    1986-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Radio telescope for millimeter wavelengths.

    FISHER, R. C. / HOARD, H. S. | AIAA | 1966


    Radio telescope for millimeter wavelengths

    FISHER, R. / HOARD, H. / ONIANS, F. | AIAA | 1964


    Apparatus for spectral radio astronomical observations at millimeter wavelengths

    Zinchenko, I.I. / Andrijanov, A.F. / Burov, A.B. et al. | IEEE | 1989


    Stellar coronal activity

    Pallavicini, R. | Online Contents | 2000


    Stellar Coronal Activity

    Pallavicini, R. / International Council of Scientific Unions | British Library Conference Proceedings | 2000