Optical spectra of the galaxy NGC 6677 and the adjacent 'bright compact object'

Details Optical spectra of the galaxy NGC 6677 and the adjacent 'bright compact object' Optical spectra of the galaxy NGC 6677 and the adjacent 'bright compact object'

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..451c&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, June 1987, p. 451-454. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Galactic Structure, Stellar Spectra, Visible Spectrum, Active Galaxies, Emission Spectra, Line Spectra, Mass Distribution, Milky Way Galaxy

Scientific paper

Spectral observations of the NGC 6677 galaxy and the adjacent object showed that: (1) the bright compact object is a star belonging to our Galaxy but not an active galaxy; (2) the NGC 6677 galaxy has a sufficiently rich emission spectrum. On the basis of measured values of Z, the inclination and the extent of emission lines, the mass of the galaxy has been estimated (M = 7×109M_sun;).

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