Continuum and reddening of the peculiar nucleus of NGC 5236

Details Continuum and reddening of the peculiar nucleus of NGC 5236 Continuum and reddening of the peculiar nucleus of NGC 5236

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..67..417d&link_type=abstract

Astrophysics and Space Science, vol. 67, no. 2, Feb. 1980, p. 417-426. Research supported by the Financiadora de Estudos e Proj

Astronomy and Astrophysics

Astrophysics

1

Continuous Radiation, Galactic Nuclei, Galactic Structure, Interstellar Extinction, Red Shift, Stellar Spectrophotometry, Ubv Spectra, Astronomical Photography, B Stars, Chemical Composition, M Stars, Stellar Structure

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Continuum and reddening of the peculiar nucleus of NGC 5236 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Continuum and reddening of the peculiar nucleus of NGC 5236, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Continuum and reddening of the peculiar nucleus of NGC 5236 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1620435