Pulsed and Continuous Radiation from White Dwarfs

Details Pulsed and Continuous Radiation from White Dwarfs Pulsed and Continuous Radiation from White Dwarfs

Jul 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..17..117l&link_type=abstract

Astrophysics and Space Science, Volume 17, Issue 1, pp.117-125

Astronomy and Astrophysics

Astrophysics

Scientific paper

We demonstrate that the detection of steady kV X-ray emission from the vicinity of a white dwarf star possessing a magnetic field of the order of 107 G will provide strong evidence that the white dwarf is rotating with a period of about one minute. We also show that detection of pulsed radiation at about 1 mm wavelength would confirm this. Also some of the interesting dynamical consequences for the interstellar medium due to such white dwarfs are outlined.

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