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Astrophysics and Space Science, 1985
In this paper we discuss observational and theoretical arguments in favour of hypothesis on ‘nomad life’ of active nuclei inside and outside galaxies as well as its consequences. It may be the anisotropic collapse of a supermassive star, or the disruption of a supermassive binary system after the collapse of one companion that would give birth to such ...
O. K. Sil'chenko, V. M. Lipunov
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In this paper we discuss observational and theoretical arguments in favour of hypothesis on ‘nomad life’ of active nuclei inside and outside galaxies as well as its consequences. It may be the anisotropic collapse of a supermassive star, or the disruption of a supermassive binary system after the collapse of one companion that would give birth to such ...
O. K. Sil'chenko, V. M. Lipunov
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Publications of the Astronomical Society of the Pacific, 1965
613 SB(rs)bc fB-fS3 AN This note 1097 SB(s)b gBp HS 2 1365 SB(s)b fgB HS 2 1433 SB(r)a gB AN This note 1672 SB(s)b fB AN This note 1808 RSAB(s)a fS5p HS 2 2997 SAB(rs)c fSl HS This note 3351 SB(r)b fgBl HS 2 4051 SAB(rs)bc f?S3N AN This note 4151 SAB(rs)ab: gkS4pN AN This note 4321 SAB(s)bc fgSl HS 2 5236 SAB(s)c fgSl AN This note 5248 SAB(rs)bc fS4 HS
J. L. Sérsic, M. Pastoriza
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613 SB(rs)bc fB-fS3 AN This note 1097 SB(s)b gBp HS 2 1365 SB(s)b fgB HS 2 1433 SB(r)a gB AN This note 1672 SB(s)b fB AN This note 1808 RSAB(s)a fS5p HS 2 2997 SAB(rs)c fSl HS This note 3351 SB(r)b fgBl HS 2 4051 SAB(rs)bc f?S3N AN This note 4151 SAB(rs)ab: gkS4pN AN This note 4321 SAB(s)bc fgSl HS 2 5236 SAB(s)c fgSl AN This note 5248 SAB(rs)bc fS4 HS
J. L. Sérsic, M. Pastoriza
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Annual Review of Astronomy and Astrophysics, 1970
Galactic nuclei activity effect on galactic evolution and cosmology, discussing stellar and gaseous ...
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Galactic nuclei activity effect on galactic evolution and cosmology, discussing stellar and gaseous ...
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Astronomische Nachrichten, 1976
AbstractThe parameters of fifteen active nuclei are determined from spectroscopic and photometric observations. The values of bolometric luminosity, gas volume and mass, kinetic energy, characteristic dimension and kinematic time‐scale are given. The fluxes of radiative and mechanical energy of the gas envelope are compared. A steady‐state model of the
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AbstractThe parameters of fifteen active nuclei are determined from spectroscopic and photometric observations. The values of bolometric luminosity, gas volume and mass, kinetic energy, characteristic dimension and kinematic time‐scale are given. The fluxes of radiative and mechanical energy of the gas envelope are compared. A steady‐state model of the
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Publications of the Astronomical Society of the Pacific, 1986
The author reviews recent research on the environment in which active nuclei reside, namely the dense stellar populations found in the centers of elliptical galaxies and spiral bulges. He discusses new developments concerning the structure and dynamics of nuclei, recent results on the age and chemical composition of nuclear populations, the possibility
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The author reviews recent research on the environment in which active nuclei reside, namely the dense stellar populations found in the centers of elliptical galaxies and spiral bulges. He discusses new developments concerning the structure and dynamics of nuclei, recent results on the age and chemical composition of nuclear populations, the possibility
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The anti-nuclei production of our galaxy
Nuclear Physics B - Proceedings Supplements, 1999Abstract The discovery of a single anti-helium nucleus in the cosmic ray flux would definitely point toward the existence of stars and even of entire galaxies made of anti-matter. The presence of anti-nuclei in cosmic rays has actually profound implications on the fundamental question of the baryon asymmetry of the universe.
Salati, P., Chardonnet, P., Orloff, Jean
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Active Galaxies And Their Nuclei
2004Abstract At a conference held in Manchester in 1984, Bernard Pagel aptly paraphrased George Orwell by commenting that”all galaxies are active, but some are more active than others.” Activity in galaxies manifests itself in a variety of ways.
T W Hartquist, J E Dyson, D P Ruffle
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MILLER-UREY SYNTHESIS IN THE NUCLEI OF GALAXIES
Astrophysics and Space Science, 1998The most promising venues for the synthesis of prebiotic molecules by Miller-Urey type processes may be found near the centres of galaxies. Explosions of supermassive stars would produce the basic chemical elements necessary to make molecules in high-density mass flows that are then acted upon by ionizing radiation, thus simulating the conditions ...
N.C. Wickramasinghe, F. Hoyle
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Recurrent Seyfert activity in spiral galaxy nuclei
Nature, 1981Hills1 has pointed out that in some conditions black holes in galactic nuclei would rapidly grow by disruption and accretion of stars thus producing Seyfert luminosities (>1043 erg s−1). In this hypothesis only those galactic nuclei with a high central stellar density are susceptible to Seyfert pathology, and they evolve through only one Seyfert phase.
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