Spectral observations of new galaxies with ultraviolet excess. II

Journal Article · Sun May 01 04:00:00 EDT 1988 · Astrophysics (Engl. Transl.); (United States)

DOI:https://doi.org/10.1007/BF01012445· OSTI ID:5875642

Kazaryan, M A

The results are given of spectral observations of 41 galaxies with ultraviolet excess. The spectra were obtained with the 6-m telescope of the Special Astrophysical Observatory with SP-160 and UAGS spectrograph in conjunction with image tubes. Emission lines are observed in the spectra of 36 galaxies; four objects, Nos. 147, 214, 323, and 336, have the features of type 2 Seyfert galaxies, and No. 238 may be a candidate for a Seyfert galaxy. No lines have been observed in the spectra of galaxies Nos. 38, 72, 122, and 184; for Nos. 38 and 184 no lines have been observed in the wide spectral intervals /lambda//lambda/ 3550-7000 /angstrom/ and 3500-7700 /angstrom/, respectively.

• Research Organization: Erevan State Univ. (USSR)
• OSTI ID: 5875642
• Journal Information: Astrophysics (Engl. Transl.); (United States), Journal Name: Astrophysics (Engl. Transl.); (United States) Vol. 27:3; ISSN ATPYA
• Country of Publication: United States
• Language: English

Related Subjects

640105* -- Astrophysics & Cosmology-- Galaxies
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ABSORPTION SPECTRA
ELECTROMAGNETIC RADIATION
ELEMENTS
EMISSION SPECTRA
FLUIDS
GALAXIES
GALAXY NUCLEI
GASES
HYDROGEN
LINE WIDTHS
LUMINOSITY
NEON
NITROGEN
NONMETALS
OPTICAL PROPERTIES
OXYGEN
PHYSICAL PROPERTIES
RADIATIONS
RARE GASES
RED SHIFT
REMOTE SENSING
SEYFERT GALAXIES
SPECTRA
ULTRAVIOLET RADIATION