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Continuum and reddening of the peculiar nucleus of NGC 5236
Photographic spectrophotometry and UBV multi-aperture photometry are used to analyze the stellar composition and gas content within a region of 12 arcsec in the nuclear bulk of the Sersic-Pastoriza galaxy NGC 5236. An internal reddening E(B - V) equals 0.2 + or - 0.1 mag. is derived for this region....
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Published in: | Astrophysics and space science 1980-02, Vol.67 (2), p.417-426 |
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Main Author: | |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Photographic spectrophotometry and UBV multi-aperture photometry are used to analyze the stellar composition and gas content within a region of 12 arcsec in the nuclear bulk of the Sersic-Pastoriza galaxy NGC 5236. An internal reddening E(B - V) equals 0.2 + or - 0.1 mag. is derived for this region. The failure of the fit between the synthetic and the observed continuum for wavelengths from 5600 to 6500 A is discussed. |
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ISSN: | 0004-640X 1572-946X |
DOI: | 10.1007/BF00642395 |