| 000 | 01999nam a22003858i 4500 | ||
|---|---|---|---|
| 001 | CR9780511564604 | ||
| 003 | UkCbUP | ||
| 005 | 20200124160238.0 | ||
| 006 | m|||||o||d|||||||| | ||
| 007 | cr|||||||||||| | ||
| 008 | 090518s1998||||enk o ||1 0|eng|d | ||
| 020 | _a9780511564604 (ebook) | ||
| 020 | _z9780521550574 (hardback) | ||
| 020 | _z9780521087834 (paperback) | ||
| 040 |
_aUkCbUP _beng _erda _cUkCbUP |
||
| 050 | 0 | 0 |
_aQB853.5 _b.A84 1998 |
| 082 | 0 | 0 |
_a523.8/55 _221 |
| 100 | 1 |
_aAshman, Keith M., _d1963- _eauthor. |
|
| 245 | 1 | 0 |
_aGlobular cluster systems / _cKeith M. Ashman, Stephen E. Zepf. |
| 264 | 1 |
_aCambridge : _bCambridge University Press, _c1998. |
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| 300 |
_a1 online resource (x, 171 pages) : _bdigital, PDF file(s). |
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| 336 |
_atext _btxt _2rdacontent |
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| 337 |
_acomputer _bc _2rdamedia |
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| 338 |
_aonline resource _bcr _2rdacarrier |
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| 490 | 1 |
_aCambridge astrophysics ; _v30 |
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| 500 | _aTitle from publisher's bibliographic system (viewed on 05 Oct 2015). | ||
| 520 | _aGlobular clusters are roughly spherical, densely packed groups of stars found around galaxies. Most globular clusters probably formed at the same time as their host galaxies. They therefore provide a unique fossil record of the conditions during the formation and early evolution of galaxies. This volume presents a comprehensive review of globular cluster systems. It summarizes their observed properties, and shows how these constrain models of the structure of stars, the formation and evolution of galaxies and globular clusters, and the age of the Universe. For graduate students and researchers, this volume provides the definitive reference on globular cluster systems. | ||
| 650 | 0 |
_aStars _xGlobular clusters. |
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| 650 | 0 |
_aGalaxies _xFormation. |
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| 650 | 0 | _aAstrophysics. | |
| 700 | 1 |
_aZepf, Stephen E., _d1963- _eauthor. |
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| 776 | 0 | 8 |
_iPrint version: _z9780521550574 |
| 830 | 0 |
_aCambridge astrophysics series ; _v30. |
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| 856 | 4 | 0 | _uhttps://doi.org/10.1017/CBO9780511564604 |
| 999 |
_c518246 _d518244 |
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