W. Hagen scite author profile

Zeeman spectroscopic observations show that HD 101065 (Przybylski's star) has a magnetic field strength of about -2200 gauss. The limited observations available show no evidence of magnetic or spectrum variability. Observations of the Am star 8 Nor were made in order to determine whether systematic errors were present in the determination of H e , and these data yield an upper limit of 150 gauss for the field of 8 Nor.

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W. Hagen

The infrared spectra of amorphous solid water and ice Ic between 10 and 140 K

Interstellar molecule formation in grain mantles: The laboratory analog experiments, results and implications

The circumstellar envelopes of M giants

Luminosities and mass loss rates of OH/H2O maser stars

The magnetic field of HD 101065.

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