Observations of NGC 604 over six decades in frequency

Details Observations of NGC 604 over six decades in frequency Observations of NGC 604 over six decades in frequency

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...105..229i&link_type=abstract

Astronomy and Astrophysics, vol. 105, no. 2, Jan. 1982, p. 229-235. Research supported by the Koninklijke Nederlandse Akademie

Astronomy and Astrophysics

Astrophysics

22

Astronomical Maps, Astronomical Spectroscopy, Galactic Structure, H Alpha Line, Radio Spectra, H Ii Regions, Infrared Spectra, Line Spectra, Near Infrared Radiation, Nebulae, Radiant Flux Density, Red Shift, Star Clusters, Ultraviolet Spectra

Scientific paper

Maps in the near-infrared, H-alpha and radio continuum have been obtained of NGC 604, the brightest H II region complex in M33, as well as a measurement of the UV spectrum of the ionizing star cluster. The data show that NGC 604 consists of about ten components of typical size 10 pc, embedded in a much larger envelope with dimensions of 225 pc. At least one component is optically almost completely obscured; it is located close to another object that is only detected in the near-infrared and whose nature is uncertain.

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