The main body of NGC 1275 in the visible ultraviolet

Details The main body of NGC 1275 in the visible ultraviolet The main body of NGC 1275 in the visible ultraviolet

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pasp...89..488a&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 89, Aug.-Sept. 1977, p. 488-490.

Other

18

Galactic Structure, Hot Stars, Image Tubes, Infrared Photography, Near Infrared Radiation, Star Distribution, Ultraviolet Photography, Astronomical Photography, Emission Spectra, Photographic Plates

Scientific paper

New image-tube direct plates of NGC 1275 in the visible ultraviolet and the near infrared are presented. The respective filters were chosen to reduce the effect of line emission and to emphasize the hot and cool stellar populations. These plates are compared with other published plates in order to study the distribution of hot stars in the main body of NGC 1275. Hot stars are found to be associated with the line-emitting knots in the high-redshift system, but not the low-redshift system. The presence of two important outlying structures that emit in the ultraviolet continuum is also discussed.

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