An exceptionally bright, compact starburst nucleus

Details An exceptionally bright, compact starburst nucleus An exceptionally bright, compact starburst nucleus

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...334..597m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 334, Nov. 15, 1988, p. 597-604.

Astronomy and Astrophysics

Astrophysics

21

Balmer Series, Compact Galaxies, Galactic Nuclei, Starburst Galaxies, Ultraviolet Spectra, Brightness Distribution, Emission Spectra, Infrared Photometry, X Ray Spectra

Scientific paper

Observations are reported of a remarkably bright (V about 13) starburst nucleus, 0833 + 652, which has been detected at radio, infrared, optical, ultraviolet, and X-ray wavelengths. Despite an observed flux at each of these wavelengths which is comparable to that of NGC 7714, often considered the 'prototypical' example of the starburst phenomenon, 0833 + 652 appears to be a previously uncataloged object. Its ease of detectability throughout the electromagnetic spectrum should make it useful for a variety of problems in the study of compact emission-line galaxies.

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