4 edition of Young Galaxies and Qso Absorption-Line Systems found in the catalog.
Young Galaxies and Qso Absorption-Line Systems
Sueli M. Viegas
Published
January 1997
by Astronomical Society of the Pacific
.
Written in English
| The Physical Object | |
|---|---|
| Format | Hardcover |
| Number of Pages | 166 |
| ID Numbers | |
| Open Library | OL8706646M |
| ISBN 10 | 1886733341 |
| ISBN 10 | 9781886733343 |
an absorption line sample of absorbing systems drawn from published works, we are able to study the relationship between gas and galaxies over the latter half of the age of the Universe. A correlation between absorbers and galaxies is detected out to separation of Mpc. This correlation is weaker than the galaxy-galaxy :// Journal: Young Galaxies and QSO Absorption-Line Systems, ASP Conference Series, Vol. , , ed. Sueli M. Viegas, Ruth Gruenwald; Reinaldo R. de Carvalho (). Proceedings of a workshop held in Santos, Brazil April , p Bibliographic Code:
We present results of an ongoing program to study the gaseous extent of galaxies and the origin of QSO absorption line systems. For \lya absorption systems, we find that absorption equivalent (2) At z less than or approximately = 1 the fraction of Ly(aplha) absorption systems-including Ly(alpha)-forest absorption systems-that arise in luminous galaxies is at least +/- and may
SAO/NASA Astrophysics Data System (ADS) Title: Analysis of the Lyman-alpha Forest in Cosmological Situations Using Voigt-Profile Decomposition Authors: Dave, R 67D. SAO/NASA Astrophysics Data System (ADS) Title: The HST Quasar Absorption Line Survey: A Census of Absorption Lines at Low Redshift Authors: Jannuzi, B. T. Journal: Young Galaxies and QSO Absorption-Line Systems, ASP Conference Series, Vol. , , ed. Sueli M. Viegas, Ruth Gruenwald; Reinaldo R. de Carvalho (). Proceedings of a workshop held in Santos, Brazil April , 91J.
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Book Review: Young galaxies and QSO absorption-line systems / Astronomical Society of the Pacific, V/abstract.
Young galaxies and QSO absorption-line systems: proceedings of a workshop held in Santos, Brazil, April They include (1) evidence for neutral hydrogen Gunn-Peterson absorption near redshift z=, (2) interpretation of the redshift evolution of the mass spectrum of interstellar hydrogen clouds in young galaxies as derived from observations of damped Ly-alpha systems Abstract.
10 m class telescopes and their instrumentation will greatly benefit the study of QSO absorption line systems. Two main subjects are discussed: the detection of the associated galaxies; and the determination of absorption line system physical properties Title: Book Review: Young galaxies and QSO absorption-line systems / Astronomical Society of the Pacific, Journal: The Observatory, vol.no.p.
() Bibliographic Code: Obs V. Complete bibliographic record Other article options Print this V. Cosmic Minivoids in the Intergalactic Medium Young Galaxies and QSO Absorption-Line Systems.
Pub Date: arXiv: arXiv:astro-ph/ Bibcode: ASPCM Keywords: Astrophysics; E-Print: Latex, 10 pages, includes 6 figures. Invited talk presented at IAGUSP Workshop on Young Galaxies and QSO Absorbers in Santos, Brazil, April PDF | OnA.
Penny and others published Book Review: PLANETARY SYSTEMS IN THE UNIVERSE - OBSERVATION, FORMATION AND EVOLUTION / Astronomical Society of the Pacific, | Find, read adshelp[at] The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86A 11P/abstract.
By studying the physical conditions in galaxies at different redshifts, we can begin to understand the evolutionary process of starformation from early epochs to the present. Such studies have been performed at optical and centimeter wavelengths for a number of years.
Due to advances in receiver and telescope technology at millimeter and submillimeter wavelengths, molecular line studies have W/abstract.
Probing galaxies through quasar absorption lines () AGN physics with the sloan digital sky survey ( Young galaxies and QSO absorption-line systems () Les noyaux actifs de galaxies () QSO absorption line meeting ( ; Baltimore, Md.) Martin John ://://cbd.
Young galaxies and QSO absorption - line systems: proceedings of a workshop held in Santos, Brazil, April, edited by Sueli M. Viegas, Ruth Gruenwald, and Reinaldo R. de Carvalho （Astronomical Society of the Pacific conference series, v. ） （A series of books on recent developments in astronomy and astrophysics, v.
） Astronomical Society of the Pacific, We propose slitless spectroscopic observations with the FOC of two luminous star-forming galaxies at z~ to determine the amplitude of their intrinsic Lyman breaks.
The opacity to ionizing UV photons of even the closest starbursts, not to mention the Milky Way, remains highly uncertain and yet bears directly on such issues as the ionization source for the Lyman-alpha forest and other QSO CiteSeerX - Document Details (Isaac Councill, Lee Giles, Pradeep Teregowda): Dwarf galaxies (DGs) are more numerous than large galaxies.
Most dwarfs in clusters are dEs, but in the field they belong mostly to late types. The importance of late-type DGs in the context of the intergalactic medium (IGM) lies in the fact that (at least some) are probably “young ” galaxies forming stars for the ?doi= Request PDF | On Jan 1,M.
Rosado and others published Book Review: Galaxies: the third dimension / Astronomical Society of the Pacific, | Find, read and cite all the research you need Common QSO Absorption Line Systems Some absorption line systems, such as HI, CII, CIV, OVI, MgII, SiIV, are more frequently detected in QSO spectra than other systems.
The reason is that the elements of these species generally have high cosmic abundances and the transitions involved have large oscillator strengths. Obsevational reasons. ~hjmo/astro/lecturepdf.
Probing galaxies through quasar absorption lines. 1) QSO absorption line background and jargon - curve of growth and Voigt profiles - naming conventions - physical motivations 2)Damped Lyman alpha systems (DLAs) properties - neutral gas content - chemical abundances - molecular gas 3)The nature of DLAs and sub-DLAs - imaging of ~sara/QAL_pdf.
line–of–sight correlations of C iv and Mg ii absorption–line systems on large scales, using an extensive catalog of heavy–element absorption–line systems in over QSO spectra (Vanden Berk et al. (More details about the catalog can be found in an earlier version of the catalog [York et al.
], as well as in QVY.) Request PDF | OnK. van der Hucht and others published Book Review: Wolf-Rayet phenomena in massive stars and starburst galaxies / Astronomical Society of the Pacific, | Find Abstract.
QSO metal-line absorption systems are reviewed in the context of galaxy formation and evolution. Attention is focused on the high column density “damped Lyα” absorption systems, which dominate the cosmological mass density of neutral gas in the universe and hence trace the bulk of material available for star formation to high redshifts Recent evidence of evolution of the gaseous T1 - Observations of nickel, chromium, and zinc in QSO absorption-line systems.
AU - Meyer, David M. AU - Roth, Katherine C. PY - /11/1. Y1 - /11/1. N2 - We present new observations of Ni II, Cr II, and Zn II in several damped Lya QSO absorption-line systems at z ≈ ://. Results relating to galaxy luminosities and impact parameters are t: 4 pages, Latex, to appear in the proceedings of the Young Galaxies and QSO Absorption-line Systems conference held in Santos, Brazil in April, SAO/NASA Astrophysics Data System (ADS) Title: Origin of Magnetic Fields Authors: Opher, R.
Journal: Young Galaxies and QSO Absorption-Line Systems, ASP Conference Series, Vol., ed. Sueli M. Viegas, Ruth Gruenwald; Reinaldo R. de Carvalho (). Proceedings of a workshop held in Santos, Brazil Aprilp Bibliographic Code: If metal-line systems occur only where the line of sight to a QSO intercepts a galaxy, we already have information on many hundreds of galaxies at redshifts greater than unity.
Here we review research on the connection between galaxies and absorption line systems seen in QSO ://
