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  • 1
    Monograph available for loan
    Monograph available for loan
    Oxford : Oxford Univ. Press
    Call number: IASS 14.0014
    Type of Medium: Monograph available for loan
    Pages: X, 550 S. : Ill., graph. Darst., Kt.
    Edition: Repr.
    ISBN: 9780199606504
    Branch Library: RIFS Library
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 257 (1997), S. 95-106 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The discussion of the problems of observation of tenuous intergalactic and/or halo clouds in recombination emission is presented. We elaborate the possibility that clouds are illuminated only by metagalactic ultraviolet radiation flux, and assume some plausible values for the parameters determining the physical conditions in such objects. A simple, semiqualitative approach may give specific observational predictions for the two major signposts of fluorescent emission: Lyα and Hα lines. We conclude that Hα detection of Lyman-limit systems at low redshift is within present observational capabilities. Open questions for further research are put in a convenient framework.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 262 (1998), S. 39-52 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The problem of influence of the ambiental intergalactic pressure on extended gas associated with normal field galaxies is briefly discussed. An empirically established characteristic radius of absorption can not be explained in the context of simple two-phase halo model as a consequence of pressure equilibrium of the hot halo with the smooth intergalactic medium. This conclusion is based upon the stringent constraints on the temperature and density of the intergalactic plasma obtained through the CMBR measurements. On the other hand, ram-pressure stripping caused by peculiar motions of galaxies does present a viable alternative for the hot halo truncation. It is shown that for a particular set of chosen parameters, a simple model is capable of producing the absolute upper limit on the extent of gas associated with the galaxy. The values obtained are compatible with the results of the recent QSO absorption-line studies, and are significantly higher than the radius at which the cooling timescale of the halo gas equates the dynamical timescale.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 274 (2000), S. 675-687 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The influence of recent detections of a finite vacuum energy(`cosmological constant') on our formulation of anthropic conjectures,particularly the so-called Final Anthropic Principle is investigated. Itis shown that non-zero vacuum energy implies the onset of a quasi-exponentialexpansion of our causally connected domain (`the universe') at some point inthe future, a stage similar to the inflationary expansion at the verybeginning of time. The transition to this future inflationary phase ofcosmological expansion will preclude indefinite survival of intelligentspecies in our domain, because of the rapid shrinking of particle horizonsand subsequent depletion of energy necessary for information processes withinthe horizon of any observer. Therefore, to satisfy the Final AnthropicHypothesis (reformulated to apply to the entire ensemble of universes), itis necessary to show that (i) chaotic inflation of Linde (or some similarmodel) provides a satisfactory description of reality, (ii) migration betweencausally connected domains within the multiverse is physically permitted, and(iii) the time interval left to the onset of the future inflationary phaseis sufficient for development of the technology necessary for suchinter-domain travel. These stringent requirements diminish the probabilityof the Final Anthropic Hypothesis being true.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 274 (2000), S. 867-875 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The discussion of the relationship between cooling radius in two-phaseadiabatic halo models and observationally established maximal radiusof absorption in luminous galaxies at low redshift is presented. It isof paramount importance that any viable model of the halo is able toreproduce empirical value of the absorption cross-section of normalgalaxies and its scaling with luminosity. Several ways for bringingthe theoretical and observational values into agreement are outlined.It is of great methodological importance to fully assess the difficultiesany model is likely to encounter when testing predicted extent ofabsorption and column density distribution against recently obtainedlow-redshift Lyα absorption data.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 271 (2000), S. 91-95 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract A simple consistency argument for hypothesis of the galactic halo origin of the Lyα forest absorption lines is advanced, based on the recent determination of column-density vs. impact parameter relation for the low-redshift gaseous galactic haloes. It is shown that observations of neutral hydrogen absorption around luminous galaxies are consistent with the index of the power-law column density distribution derived from statistical analyses of large samples of high-redshift Lyα forest lines.PACS: 98.62.Ra, 98.62.Gq, 98.80.Es
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 262 (1998), S. 497-508 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract If a significant fraction of QSO absorption line systems arises in halos of normal galaxies, absorber statistical data will tell us a lot about the structure of the gaseous envelopes of galaxies. Comparison of a class of density profile models for the metal-absorbing halos of luminous galaxies with the recent Lyα empirical data is presented. Cosmological mass fraction contained in such gas is also briefly discussed. It is shown that important constraints on the model parameters can be inferred in this way.
    Type of Medium: Electronic Resource
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  • 8
    Publication Date: 2018
    Description: 〈div data-abstract-type="normal"〉〈p〉Recent paper by Robert Klee in this journal argues that we should endorse a form of cosmic pessimism due to the inevitable destruction of Earth and humanity, allegedly meaning the complete and total annihilation of all traces of humanity's existence (‘human expunction’). It could be shown that both the physical basis and philosophical methodology used by Klee to reach those bleak conclusions are at best premature and at worst unwarranted and misleading. Even worse, they reflect a mindset of unjustified and narrow-minded technological and societal pessimism, which contributes to the erosion of the Enlightenment values, the loss of public interest in space research and colonization, and could indeed increase vulnerability to real – as opposed to uncertain eschatological – global risks humanity is facing in this millennium.〈/p〉〈/div〉
    Print ISSN: 1473-5504
    Electronic ISSN: 1574-3006
    Topics: Biology , Geosciences
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  • 9
    Publication Date: 2017-11-01
    Print ISSN: 0265-9646
    Electronic ISSN: 1879-338X
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics , Political Science
    Published by Elsevier
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  • 10
    Publication Date: 2013-08-17
    Print ISSN: 0169-3867
    Electronic ISSN: 1572-8404
    Topics: Biology , Philosophy
    Published by Springer
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