Spectroscopy of Stellar‐like Objects Contained in the Second Byurakan Survey. I

The results of spectroscopic observations of 363 starlike objects from the Second Byurakan Survey (SBS) are reported. This SBS subsample has proved to be a rich source of newly identified quasars, Seyfert‐type galaxies, degenerate stars, and hot subdwarfs. In the subsample studied here, we identifie...

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Veröffentlicht in:Publications of the Astronomical Society of the Pacific 1999-09, Vol.111 (763), p.1099-1114
Hauptverfasser: Stepanian, J. A., Chavushyan, V. H., Carrasco, L., Tovmassian, H. M., Erastova, L. K.
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container_title Publications of the Astronomical Society of the Pacific
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creator Stepanian, J. A.
Chavushyan, V. H.
Carrasco, L.
Tovmassian, H. M.
Erastova, L. K.
description The results of spectroscopic observations of 363 starlike objects from the Second Byurakan Survey (SBS) are reported. This SBS subsample has proved to be a rich source of newly identified quasars, Seyfert‐type galaxies, degenerate stars, and hot subdwarfs. In the subsample studied here, we identified 35 new QSOs, 142 white dwarfs (the majority of which, 114, are of DA type), 55 subdwarfs (29 of which are sdB‐type stars), 10 horizontal‐branch blue stars, 16 normal or horizontal‐branch stars, 54 G‐type and 25 F‐type stars, two objects with composite spectra, four cataclysmic variables, two peculiar emission‐line stars, 17 objects with continuous spectra, as well as one planetary nebula. Among the 35 QSOs, we have found two broad absorption line (BAL) QSOs, namely, SBS 1423+500 and SBS 1435+500A. Magnitudes, redshifts, and slit spectra for all QSOs, and also some typical spectra of the peculiar stars, are presented. We estimate the minimum surface density of bright QSOs in the redshift range \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $0.3< z< 2.2$ \end{document} to be 0.05 deg−2for \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $B< 17$ \end{document} .0 mag and 0.10 deg−2for \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcom
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Among the 35 QSOs, we have found two broad absorption line (BAL) QSOs, namely, SBS 1423+500 and SBS 1435+500A. Magnitudes, redshifts, and slit spectra for all QSOs, and also some typical spectra of the peculiar stars, are presented. 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source IOP Publishing Journals; JSTOR Archive Collection A-Z Listing; EZB-FREE-00999 freely available EZB journals; Institute of Physics (IOP) Journals - HEAL-Link; Alma/SFX Local Collection
subjects Astronomical objects
Emission spectra
Peculiar stars
Quasars
Red shift
Stellar classification
Stellar spectra
Subdwarf stars
Telescopes
Wavelengths
title Spectroscopy of Stellar‐like Objects Contained in the Second Byurakan Survey. I
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