MARC Record from harvard_bibliographic_metadata

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005 20131206200545.0
008 121227s1997 ne | s ||0| 0|eng d
020 $a9789401152440
020 $a9789401152440
020 $a9780792348931
024 7 $a10.1007/978-94-011-5244-0$2doi
035 $a(Springer)9789401152440
040 $aSpringer
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072 7 $aPG$2bicssc
072 7 $aSCI004000$2bisacsh
072 7 $aNAT033000$2bisacsh
082 04 $a520$223
100 1 $aHabing, H. J.,$eeditor.
245 10 $aPlanetary Nebulae :$bProceeding of the 180th Symposium of the International Astronomical Union, Held in Groningen, The Netherlands, August, 26–30, 1996 /$cedited by H. J. Habing, H. J. G. L. M. Lamers.
246 3 $aProceedings of the 180th Symposium of the International Astronomical Union, held in Groningen, The Netherlands, August 26-30, 1996
264 1 $aDordrecht :$bSpringer Netherlands :$bImprint: Springer,$c1997.
300 $aXXXVIII, 507 p.$bonline resource.
336 $atext$btxt$2rdacontent
337 $acomputer$bc$2rdamedia
338 $aonline resource$bcr$2rdacarrier
347 $atext file$bPDF$2rda
490 1 $aInternational Astronimical Union / Union Astronomique Internationale ;$v180
520 $aPlanetary nebulae present a fascinating range of shapes and morphologies. They are ideal laboratories for the study of different astrophysical processes: atomic physics, radiative transfer, stellar winds, shocks, wind-wind interaction, and the interaction between stellar winds and the interstellar medium. In addition, planetary nebulae provide information about the late stages of stellar evolution. In the last five years studies of planetary nebulae have progressed very rapidly and new phenomena and insights have been gained. This is partly due to new observations (e.g. from the Hubble Space Telescope, the ISO satellite and new infrared and millimeter spectrographs) and partly to the advancement of hydrodynamic simulations of the structures of planetary nebulae (PN). Many of these new results were reported at IAU Symposium 180 in Groningen, the Netherlands, on August 26 to 30, 1996. This symposium was dedicated to one of the pioneers of PN research: Stuart Pottasch. These proceedings contain chapters on: Introduction to PN with the basic parameters Distances of PN The central stars of PN The envelopes of PN The evolution from AGB to PN The evolution from PN to white dwarfs PN in the galactic context PN in extragalactic systems The future of PN research . The book contains 29 reviews and more than 200 shorter contributions.
650 10 $aPhysics.
650 0 $aPhysics.
650 24 $aAstronomy, Observations and Techniques.
650 24 $aAstrophysics and Astroparticles.
700 1 $aLamers, H. J. G. L. M.,$eeditor.
776 08 $iPrinted edition:$z9780792348931
830 0 $aInternational Astronimical Union / Union Astronomique Internationale ;$v180.
988 $a20131114
906 $0VEN