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Titlebook: QSO Absorption Lines; Proceedings of the E Georges Meylan Conference proceedings 1995 Springer-Verlag Berlin Heidelberg 1995 Absorbing Syst

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書目名稱QSO Absorption Lines
副標(biāo)題Proceedings of the E
編輯Georges Meylan
視頻videohttp://file.papertrans.cn/781/780022/780022.mp4
叢書名稱ESO Astrophysics Symposia
圖書封面Titlebook: QSO Absorption Lines; Proceedings of the E Georges Meylan Conference proceedings 1995 Springer-Verlag Berlin Heidelberg 1995 Absorbing Syst
描述The controversial question of whether the majority of the narrow absorption lines observed in QSO spectra represent cosmological intervening systems or ejecta from the QSO themselves is settled. QSO absorption line spectroscopy, initially a mere technique, has matured into an essential extragalactic research tool for understanding the content of the Universe at redshifts between 0 and 4, and beyond. The only previous important meeting devoted to "QSO Absorption Lines" was held in May 1987 at the Space Telescope Science Institute in Baltimore, Maryland, U.S.A. Since that time, nearly a decade ago, research has been ex- tremely active in this now well-established field of astrophysics. Theoretical stud- ies and simulations have taken advantage of the constant progress in computer technology, and during these last few years, the observational results have bene- fited largely from the new facillities offered by the Hubble Space Telescope in the UV wavelength range and the Keck Telescope for high-resolution spectroscopy.
出版日期Conference proceedings 1995
關(guān)鍵詞Absorbing Systems; Absorption Lines; Abundances; BAL QSOs; Damped Lyman-alpha Systems; Large-Scale Struct
版次1
doihttps://doi.org/10.1007/978-3-540-49458-4
isbn_softcover978-3-662-22373-4
isbn_ebook978-3-540-49458-4Series ISSN 1431-2433 Series E-ISSN 1611-6143
issn_series 1431-2433
copyrightSpringer-Verlag Berlin Heidelberg 1995
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Consequences of Dust in Damped Lyman-Alpha Systemstion of Cr relative to Zn. Both methods give a typical dust-to-gas ratio roughly 10% of that in the Milky Way. Here, we review some of the consequences of these observations. First, the dust in damped Ly. systems causes obscuration and hence incompleteness in optically selected samples of quasars. W
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The Mass Spectrum of Giant Hydrogen Clouds Associated with Damped Ly, Absorberswn and nearby galaxies shows that these absorbers may be interpreted as giant hydrogen clouds (GHCs) in intervening galaxies along the lines-of-sight. We show that the observational data on the redshift and column density distribution of the DLAs may be used to study the mass spectrum of GHCs and it
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A Damped Ly, Survey at , < 1.65damped Ly. systems studied so far are found to have corresponding MgII absorption. From known MgII absorption-line statistics, we determine an upper limit to the number of damped Ly. systems per unit redshift, ..., at <.> ≈ 0.8 that is consistent with the trend at higher redshift as well as the numb
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