Spectrophotometry of the galaxies Markaryan 367, 449, and 1119

Details Spectrophotometry of the galaxies Markaryan 367, 449, and 1119 Spectrophotometry of the galaxies Markaryan 367, 449, and 1119

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....26..399b&link_type=abstract

(Astrofizika, vol. 26, May-June 1987, p. 399-403) Astrophysics (ISSN 0571-7132), vol. 26, no. 3, Nov. 1987, p. 241-244. Translat

Astronomy and Astrophysics

Astrophysics

1

Abundance, Astronomical Spectroscopy, Emission Spectra, Galactic Nuclei, Line Spectra, Markarian Galaxies, Compact Galaxies, Ionized Gases, Nitrogen, Oxygen, Spectrophotometry, Spiral Galaxies, Star Formation

Scientific paper

Spectra obtained with the 6-m telescope of the Special Astrophysical Observatory have been used to make a spectrophotometric investigation of the central regions of the galaxies Mar. 367, 449, and 1119. The relative intensities of the emission lines have been used to estimate Te and ne, the abundances of the elements O and N, the masses and volumes of ionized gas, and the number of 07 stars. The galaxy Mark. 1119 recalls blue compact galaxies with a powerful burst of star formation. The central regions of Mark. 367 and 449 have the characteristics of the nuclei of spiral galaxies with a burst of star formation.

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