For 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 ...
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For 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.
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Seller's Description:
Fine. Trade paperback (US). Glued binding. 256 p. Contains: Unspecified, Illustrations, black & white. Lecture Notes in Physics, 316. In Stock. 100% Money Back Guarantee. Brand New, Perfect Condition, allow 4-14 business days for standard shipping. To Alaska, Hawaii, U.S. protectorate, P.O. box, and APO/FPO addresses allow 4-28 business days for Standard shipping. No expedited shipping. All orders placed with expedited shipping will be cancelled. Over 3, 000, 000 happy customers.
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Seller's Description:
New. Trade paperback (US). Glued binding. 256 p. Contains: Unspecified, Illustrations, black & white. Lecture Notes in Physics, 316. In Stock. 100% Money Back Guarantee. Brand New, Perfect Condition, allow 4-14 business days for standard shipping. To Alaska, Hawaii, U.S. protectorate, P.O. box, and APO/FPO addresses allow 4-28 business days for Standard shipping. No expedited shipping. All orders placed with expedited shipping will be cancelled. Over 3, 000, 000 happy customers.
Choose your shipping method in Checkout. Costs may vary based on destination.
Seller's Description:
Fine. Trade paperback (US). Glued binding. 256 p. Contains: Unspecified, Illustrations, black & white. Lecture Notes in Physics, 316. In Stock. 100% Money Back Guarantee. Brand New, Perfect Condition, allow 4-14 business days for standard shipping. To Alaska, Hawaii, U.S. protectorate, P.O. box, and APO/FPO addresses allow 4-28 business days for Standard shipping. No expedited shipping. All orders placed with expedited shipping will be cancelled. Over 3, 000, 000 happy customers.
Choose your shipping method in Checkout. Costs may vary based on destination.
Seller's Description:
New. Trade paperback (US). Glued binding. 256 p. Contains: Unspecified, Illustrations, black & white. Lecture Notes in Physics, 316. In Stock. 100% Money Back Guarantee. Brand New, Perfect Condition, allow 4-14 business days for standard shipping. To Alaska, Hawaii, U.S. protectorate, P.O. box, and APO/FPO addresses allow 4-28 business days for Standard shipping. No expedited shipping. All orders placed with expedited shipping will be cancelled. Over 3, 000, 000 happy customers.
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Seller's Description:
Near fine in none as issued jacket. About fine, first edition, first printing. Brown, mustard and white cloth boards. Binding is sturdy, square and tight. Previous owner's name stamped neatly on top edge, otherwise as new. No dust jacket as issued. Illustrated with formulas, b/w photos, graphs, and drawings. xiii, 252 [4] pp. Octavo, 6 1/2 x 9 3/4 inches tall. For 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. ---Publisher's web site Interpretation of Supernova Shells W. Kundt Evolution of the morphology of supernova remnants with pulsars G. Srinivasan, D. Bhattacharya On the distances of the remnants of historical type I supernovae Richard G. Strom Spectral index variations in supernova remnants E. Fürst, W. Reich Statistical studies of SNRs: Selection effects D. A. Green The Galactic distribution of radio supernova remnants Sidney van den Bergh Statistical properties of recently new identified supernova remnants W. Reich, E. Fürst X-ray observations and non-equilibrium ionisation of supernova remnants W. Brinkmann Shock-cloud interactions in supernova remnants S. A. E. G. Falle, J. R. Giddings Interpretation difficulties of SNR shock spectra D. E. Innes The origin of Kepler's supernova remnant Rino Bandiera CTB80: The supernova remnant with (almost) everything Richard G. Strom G316.3-0.0 and G332A+0.1 — Two supernova remnants with blowouts D. K. Milne, J. L. Caswell, M. J. Kesteven, R. F. Haynes, R. S. Roger Puppis a and its environment as revealed by infrared observations Richard G. Arendt, Eli Dwek, Robert Petre High resolution radio observations of G11.2-0.3 D. A. Green G70.7 + 1.2: Supernova remnant? M. de Muizon, R. G. Strom, M. J. A. Oort, J. J. Claas, R. Braun A molecular cloud in the direction of G70.68+1.20 W. Reich, N. Junkes, E. Fürst Detection of four supernova remnants in the polarized emission from the Effelsberg 11 cm survey N. Junkes, E. Fürst, W. Reich Kinematics of optical filaments in the Cygnus Loop H. Greidanus, R. G. Strom X-ray observations of the supernova remnant G292.0+1.8 J. J. Claas Recent results from supernova calculations James M. Lattimer Supernova structure and light curves W. Kundt What are the masses of SNIb progenitors? Sidney van den Bergh Type Ib supernovae: What they may be and what they are not Nino Panagia, Victoria G. Laidler Ultraviolet observations of SN 1987A Nino Panagia X rays from SN 1987A: A partially obscured plerion Rino Bandiera, Franco Pacini, Marco Salvati Supernova VLBI Norbert Bartel The compact radio sources in the galaxy M82-Supernova-remnants and/or recent supernovae-Peter L. Biermann The supershells of the large magellanic cloud and their importance for the interstellar medium J. Spicker, J. V. Feitzinger Extended onion-shell model for cosmic ray spectra produced by supernova remnants L. A. Zank, H. J. Völk.
![Supernova Shells and Their Birth Events: Proceedings of a Workshop Held at the Physikzentrum Bad Honnef, March 7-11, 1988 [Lecture Notes in Physics 316]](https://www3.alibris-static.com/imageid/2033969194_t.jpg)
