| 000 | 03282nam a22004935i 4500 | ||
|---|---|---|---|
| 001 | 978-3-540-39282-8 | ||
| 003 | DE-He213 | ||
| 005 | 20190213151132.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 121227s1988 gw | s |||| 0|eng d | ||
| 020 |
_a9783540392828 _9978-3-540-39282-8 |
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| 024 | 7 |
_a10.1007/BFb0034541 _2doi |
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| 050 | 4 | _aQB4 | |
| 072 | 7 |
_aPG _2bicssc |
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_aSCI004000 _2bisacsh |
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_a520 _223 |
| 245 | 1 | 0 |
_aAtmospheric Diagnostics of Stellar Evolution: Chemical Peculiarity, Mass Loss, and Explosion _h[electronic resource] : _bProceedings of the 108th Colloquium of the International Astronomical Union, Held at the University of Tokyo, Japan, 1–4 September 1987 / _cedited by Ken'ichi Nomoto. |
| 264 | 1 |
_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c1988. |
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| 300 |
_aXIV, 468 p. 17 illus. _bonline resource. |
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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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| 347 |
_atext file _bPDF _2rda |
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| 490 | 1 |
_aLecture Notes in Physics, _x0075-8450 ; _v305 |
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| 505 | 0 | _aContents: Chemical Peculiarities as Probe of Stellar Evolution: Main-Sequence Stars. Cool Evolved Stars. Hot Evolved Stars -- Mass-Losing Stars In Different Stages of Evolution: Hot Stars. Cool Stars. Interacting Binaries -- Chemical and Dynamical Structures of Exploding Stars: Novae And Dwarf Novae. Supernovae -- Concluding Remarks -- List of Participants. | |
| 520 | _aThis collection of papers describes the evolutionary path of stars of various masses. Observational data and theoretical modeling of the stellar atmosphere and the stellar interior and their interaction are presented, covering chemical peculiarities, mass loss, and explosion, all of which are strongly related to the hydrodynamic evolution of the interior. In particular the supernova SN 1987 A is discussed for the first time in detail, including the underground neutrino observations and the detection of X-rays from the supernova. The study of its progenitor, a B 3 supergiant, was related to the topics of chemical peculiarities and mass loss mechanisms and atmospheric models. The intended readers are professional astronomers and astrophysicists, as well as physicists. The book will also be an important source of information for graduate students. | ||
| 650 | 0 | _aPhysical geography. | |
| 650 | 1 | 4 |
_aAstronomy, Observations and Techniques. _0http://scigraph.springernature.com/things/product-market-codes/P22014 |
| 650 | 2 | 4 |
_aAstrophysics and Astroparticles. _0http://scigraph.springernature.com/things/product-market-codes/P22022 |
| 650 | 2 | 4 |
_aGeophysics/Geodesy. _0http://scigraph.springernature.com/things/product-market-codes/G18009 |
| 700 | 1 |
_aNomoto, Ken'ichi. _eeditor. _4edt _4http://id.loc.gov/vocabulary/relators/edt |
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| 710 | 2 | _aSpringerLink (Online service) | |
| 773 | 0 | _tSpringer eBooks | |
| 776 | 0 | 8 |
_iPrinted edition: _z9783662137017 |
| 776 | 0 | 8 |
_iPrinted edition: _z9783662137000 |
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_iPrinted edition: _z9783540194781 |
| 830 | 0 |
_aLecture Notes in Physics, _x0075-8450 ; _v305 |
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| 856 | 4 | 0 | _uhttps://doi.org/10.1007/BFb0034541 |
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