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Cosmic Chemical Evolution - K. Nomoto
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K. Nomoto:

Cosmic Chemical Evolution - Taschenbuch

2002, ISBN: 1402004494

ID: 11518546251

[EAN: 9781402004490], Neubuch, [PU: Springer Mrz 2002], Science|Astronomy, Science|Astrophysics & Space Science, Science|Cosmology, This item is printed on demand - Print on Demand Titel. Neuware - The open cluster NGC 6791 is now considered both the oldest and the most metal-rich known. Its age is 8 -10 Gyrs, twice as old as the canonical solar-metallicity cluster M67 (Garnavich et al. 1994; Demarque, Green, & Guenther 1992; Tripicco et al. 1995). That its metallicity is significantly above solar is suggested from moderate-resolution spectroscopy and from a mismatch of its color-magnitude diagram (CMD) with solar-metallicity isochrones. Tripicco et al. (1995) find [Fe/H] = +0.27 to +0.44. The cluster population is rich. In addition to about a dozen red giants and two dozen red horizontal-branch stars, the cluster has several very hot HB stars (Kaluzny & Udalski 1992). Liebert et al. (1994) have shown that the extremely blue stars are mostly sdB/sdO stars and at least 3 or 4 are likely cluster members, the first ever discovered in an open cluster. These may provide the key to the puzzling upturn in ultraviolet flux below 1500A seen in many high-metallicity systems (Burstein et al. 1988; Ferguson et al. & Liebert 1993). 256 pp. Englisch

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Proceedings of the 187th Symposium of the International Astronomical Union, held in Kyoto, Japan, August 26-30, 1997 The open cluster NGC 6791 is now considered both the oldest and the most metal-rich known. Its age is 8 -10 Gyrs, twice as old as the canonical solar-metallicity cluster M67 (Garnavich et al. 1994; Demarque, Green, & Guenther 1992; Tripicco et al. 1995). That its metallicity is significantly above solar is suggested from moderate-resolution spectroscopy and from a mismatch of its color-magnitude diagram (CMD) with solar-metallicity isochrones. Tripicco et al. (1995) find [Fe/H] = +0.27 to +0.44. The cluster population is rich. In addition to about a dozen red giants and two dozen red horizontal-branch stars, the cluster has several very hot HB stars (Kaluzny & Udalski 1992). Liebert et al. (1994) have shown that the extremely blue stars are mostly sdB/sdO stars and at least 3 or 4 are likely cluster members, the first ever discovered in an open cluster. These may provide the key to the puzzling upturn in ultraviolet flux below 1500A seen in many high-metallicity systems (Burstein et al. 1988; Ferguson et al. & Liebert 1993). Bücher / Fremdsprachige Bücher / Englische Bücher 978-1-4020-0449-0, Springer

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The open cluster NGC 6791 is now considered both the oldest and the most metal-rich known. Its age is 8 -10 Gyrs, twice as old as the canonical solar-metallicity cluster M67 (Garnavich et al. 1994; Demarque, Green, & Guenther 1992; Tripicco et al. 1995). That its metallicity is significantly above solar is suggested from moderate-resolution spectroscopy and from a mismatch of its color-magnitude diagram (CMD) with solar-metallicity isochrones. Tripicco et al. (1995) find [Fe/H] = +0.27 to +0.44. The cluster population is rich. In addition to about a dozen red giants and two dozen red horizontal-branch stars, the cluster has several very hot HB stars (Kaluzny & Udalski 1992). Liebert et al. (1994) have shown that the extremely blue stars are mostly sdB/sdO stars and at least 3 or 4 are likely cluster members, the first ever discovered in an open cluster. These may provide the key to the puzzling upturn in ultraviolet flux below 1500A seen in many high-metallicity systems (Burstein et al. 1988; Ferguson et al. & Liebert 1993). Proceedings of the 187th Symposium of the International Astronomical Union, held in Kyoto, Japan, August 26-30, 1997 Buch (fremdspr.) Bücher>Fremdsprachige Bücher>Englische Bücher, Springer

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ISBN: 9781402004490

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K. Nomoto (Editor), J.W. Truran (Editor), K.W. Truran (Editor),Paperback - Softcover reprint of the original 1st ed. 2002,Series: International Astronomical Union Symposia Series 187, English-language edition, Pub by Springer Netherlands Books, Medicine~~General, Cosmic-Chemical-Evolution~~K-Nomoto, , , , , , , , , , Springer Netherlands

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K. Nomoto; James W. Truran:
Cosmic Chemical Evolution - Taschenbuch

2002, ISBN: 9781402004490

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Softcover reprint of the original 1st ed. 2002, Softcover, Buch, [PU: Kluwer Academic Publishers]

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Cosmic Chemical Evolution
Autor:

Nomoto, K.

Titel:

Cosmic Chemical Evolution

ISBN-Nummer:

1402004494

The IAU Symposium papers collected in this volume address virtually all aspects of the problem of nucleosynthesis, galactic chemical evolution, and cosmic chemical evolution. Discussions on theoretical models as well as observational studies are included. Theoretical models of nucleosynthesis in the Big Bang, in the first stellar generations, and in stars and supernovae over the histories of our Galaxy and other galaxies provide a measure of element production over the lifetime of the Universe. Observational studies of abundances in stars, galaxies, gas concentrations in galaxies and clusters of galaxies, the intergalactic medium, and gas clouds at high redshift are reviewed.

Detailangaben zum Buch - Cosmic Chemical Evolution


EAN (ISBN-13): 9781402004490
ISBN (ISBN-10): 1402004494
Taschenbuch
Erscheinungsjahr: 2002
Herausgeber: SPRINGER VERLAG GMBH
256 Seiten
Gewicht: 0,408 kg
Sprache: eng/Englisch

Buch in der Datenbank seit 17.10.2007 09:17:11
Buch zuletzt gefunden am 26.11.2016 12:52:36
ISBN/EAN: 1402004494

ISBN - alternative Schreibweisen:
1-4020-0449-4, 978-1-4020-0449-0

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