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020 _a9783540460015
_9978-3-540-46001-5
024 7 _a10.1007/3-540-50435-4
_2doi
050 4 _aQB4
072 7 _aPG
_2bicssc
072 7 _aSCI004000
_2bisacsh
072 7 _aPG
_2thema
082 0 4 _a520
_223
245 1 0 _aSupernova Shells and Their Birth Events
_h[electronic resource] :
_bProceedings of a Workshop Held at the Physikzentrum Bad Honnef March 7–11, 1988 /
_cedited by Wolfgang Kundt.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg,
_c1988.
300 _aVIII, 256 p. 57 illus.
_bonline resource.
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
347 _atext file
_bPDF
_2rda
490 1 _aLecture Notes in Physics,
_x0075-8450 ;
_v316
505 0 _aInterpretation of Supernova Shells -- Evolution of the morphology of supernova remnants with pulsars -- On the distances of the remnants of historical type I supernovae -- Spectral index variations in supernova remnants -- Statistical studies of SNRs: Selection effects -- The Galactic distribution of radio supernova remnants -- Statistical properties of recently new identified supernova remnants -- X-ray observations and non-equilibrium ionisation of supernova remnants -- Shock-cloud interactions in supernova remnants -- Interpretation difficulties of SNR shock spectra -- The origin of Kepler's supernova remnant -- CTB80: The supernova remnant with (almost) everything -- G316.3-0.0 and G332A+0.1 — Two supernova remnants with blowouts -- Puppis a and its environment as revealed by infrared observations -- High resolution radio observations of G11.2-0.3 -- G70.7 + 1.2: Supernova remnant? -- A molecular cloud in the direction of G70.68+1.20 -- Detection of four supernova remnants in the polarized emission from the Effelsberg 11 cm survey -- Kinematics of optical filaments in the Cygnus Loop -- X-ray observations of the supernova remnant G292.0+1.8 -- Recent results from supernova calculations -- Supernova structure and light curves -- What are the masses of SNIb progenitors? -- Type Ib supernovae: What they may be and what they are not -- Ultraviolet observations of SN 1987A -- X rays from SN 1987A: A partially obscured plerion -- Supernova VLBI -- The compact radio sources in the galaxy M82 - Supernova-remnants and/or recent supernovae - -- The supershells of the large magellanic cloud and their importance for the interstellar medium -- Extended onion-shell model for cosmic ray spectra produced by supernova remnants -- Epilogue.
520 _aFor a better understanding of supernova explosions the contributors to this volume provide researchers and graduate students in astrophysics with a broad spectrum of alternatives. The confrontation of different theories in one volume should prompt further exploration of the driving piston for the explosions and deeper understanding of the experimental data. Properties of supernova shells are discussed, such as their kinematics, ages, sizes, temperatures, spectra, polarizations, energetics and morphologies. Special attention is given to a few shells of extreme age, viz. G 70.68+1.20, Kepler's SN, and CTB 80, as well as to their statistics.
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 _aKundt, Wolfgang.
_eeditor.
_4edt
_4http://id.loc.gov/vocabulary/relators/edt
710 2 _aSpringerLink (Online service)
773 0 _tSpringer eBooks
776 0 8 _iPrinted edition:
_z9783662136478
776 0 8 _iPrinted edition:
_z9783662136461
776 0 8 _iPrinted edition:
_z9783540504351
830 0 _aLecture Notes in Physics,
_x0075-8450 ;
_v316
856 4 0 _uhttps://doi.org/10.1007/3-540-50435-4
912 _aZDB-2-PHA
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