The dwarf emission galaxy He2-10

Details The dwarf emission galaxy He2-10 The dwarf emission galaxy He2-10

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.177...91a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 177, Oct. 1976, p. 91-97.

Astronomy and Astrophysics

Astronomy

108

Galactic Radiation, Interstellar Matter, Galactic Radio Waves, Graphs (Charts), Infrared Astronomy, Nonthermal Radiation, Radiant Flux Density, Radio Astronomy, Spectrum Analysis, Wolf-Rayet Stars

Scientific paper

Optical, infrared, and radio observations of He2-10 are presented. Originally classified as a planetary nebula, He2-10 is shown to be a dwarf emission galaxy with a nonthermal radio continuum. Features resembling Wolf-Rayet bands are present in the spectrum. The galaxy is particularly rich in neutral hydrogen and radiates most of its energy in the infrared.

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