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  • ASTROPHYSICS  (2)
  • 1990-1994  (2)
  • 1993  (2)
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  • 1990-1994  (2)
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  • 1
    Publication Date: 2019-08-28
    Description: Lick Observatory slit spectra of 38 objects which were claimed to have pronounced UV excess and emission lines are presented. Eleven QSOs, four galaxies at z of about 0.1, 22 stars, and one unidentified object with a low S/N spectrum were found. Of 11 objects which Zhan and Chen (1987, 1989) suggested were QSO with z(prism) not greater than 2.8; eight are QSOs. Six of the QSOs show absorption systems, including Q0000+027A with a relatively strong associated C IV absorption system, and Q0008+008 with a damped Ly-alpha system with an H I column density of 10 exp 21/sq cm. The equivalent widths of the Ca II K line, the G band, and the Balmer lines in 10 stars with the best spectra are measured, and metallicities are derived. Seven of them are in the range -2.5 to -1.7, while the others are less metal-poor.
    Keywords: ASTROPHYSICS
    Type: Astronomical Journal (ISSN 0004-6256); 106; 2; p. 426-443.
    Format: text
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  • 2
    Publication Date: 2019-07-13
    Description: The detection of a bright Fe II 12567-A forbidden line from the central regions of NGC 1275 is reported. The intensity of the Fe II 12567-A forbidden line relative to that of the other emission lines indicates the presence of a high abundance of iron in the gas phase, while the narrow width of the feature implies an origin outside the active nucleus. While a power-law continuum from the nucleus or from the cooling flows could excite the Fe II forbidden line emission, neither offers a likely mechanism for processing the circumnuclear dust grains in NGC 1275. This is not the case for shocks, which can also produce the low-ionization features characteristic of many of the off-nucleus emission line regions of NGC 1275.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 414; 2; p. 527-534.
    Format: text
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