The nucleus of the Milky Way is known to harbour regions of intense star formation activity as well as a supermassive black hole. Recent observations have revealed regions of γ-ray emission reaching far above and below the Galactic Centre (relative to the Galactic plane), the so-called 'Fermi bubbles'. It is uncertain whether these were generated by nuclear star formation or by quasar-like outbursts of the central black hole and no information on the structures' magnetic field has been reported.
View Article and Find Full Text PDFThe interstellar medium of the Milky Way is multiphase, magnetized and turbulent. Turbulence in the interstellar medium produces a global cascade of random gas motions, spanning scales ranging from 100 parsecs to 1,000 kilometres (ref. 4).
View Article and Find Full Text PDFWe have measured the Faraday rotation toward a large sample of polarized radio sources behind the Large Magellanic Cloud (LMC) to determine the structure of this galaxy's magnetic field. The magnetic field of the LMC consists of a coherent axisymmetric spiral of field strength approximately 1 microgauss. Strong fluctuations in the magnetic field are also seen on small (<0.
View Article and Find Full Text PDFFor 176 postmenopausal women on HRT with progestogen addition 'on demand' medroxyprogesterone acetate (MPA), noresthisterone and tibolone were used to protect the endometrium in 214 cases. Tibolone is a gonadomimetic steroid with combined progestogenic and estrogenic effects. In this study tibolone has been used as a progestogen.
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