Astronomers using the Wisconsin H-Alpha Mapper tool (WHAM) found that ionized hydrogen in our galaxy The Milky Way is located not only in the vicinity of the stars, but also at a relatively large distance from them.
In the late 1970’s. Astrophysicist Ron Reynolds of the University of Wisconsin in Madison, USA, sent a specially designed spectrometer to the sky and discovered a phenomenon that had not previously been observed-the reddish glow of ionized hydrogen in interstellar space. Later Reynolds and his colleagues developed the WHAM tool, a spectrometer capable of recording this dim, diffuse light emanating from interstellar space.
In the new work, scientists using the tool WHAM published the most detailed map to date of ionized hydrogen filling the Milky Way galaxy. Now known to astrophysicists as the “Reynolds layer”, this structure, 75,000 light-years in diameter and 6,000 light-years in thickness, is located in the plane of the galaxy and rotates with it.
An important finding made by researchers in this work was the elucidation of the role of certain stars in the ionization of hydrogen within our galaxy. As it turned out, for the ionization of all the observed hydrogen, it is required that its ionization occurs not only in the immediate vicinity of bright stars of the spectral class O, which play an important role in the ionization of hydrogen, but also at a relatively large distance from them, far from the star-forming regions, in the depth of which they Are usually located.