2010, ISBN: 3642082459

[EAN: 9783642082450], Neubuch, [SC: 0.0], [PU: Springer Berlin Heidelberg], PLANET; ASTROELECTRON; EVOLUTION; HYDROGEN; MAGNETICFIELD; MAGNETICFIELDS; NEBULA; PHOTON; RADIATION; SPECTRA; … Mehr…

[EAN: 9783642082450], Neubuch, [SC: 0.0], [PU: Springer Berlin Heidelberg], PLANET; ASTROELECTRON; EVOLUTION; HYDROGEN; MAGNETICFIELD; MAGNETICFIELDS; NEBULA; PHOTON; RADIATION; SPECTRA; TEMPERATURE; TRANSLATION; ULTRAVIOLET, Druck auf Anfrage Neuware - Printed after ordering - Planetary nebulae are the classic subject of astrophysics. The physical pro cesses occurring in this highly ionized gaseous medium, the formation of emis sion lines in clearly specified conditions, the continuous emission extending from the far ultraviolet up to infrared and radio frequencies, the generation of exotic forms of radiation predicted by atomic physics, along with methods for deciphering the observed spectra and detecting physical and kinematic parameters of the radiating medium, etc. - all these problems form the solid foundations of the physical theory of gaseous nebulae. They are an essential part of the arsenal of powerful tools and concepts without which one cannot imagine understanding and interpreting the enormous diversity of processes taking place in the Universe - in gaseous envelopes surrounding the stars of various classes, from cool dwarfs and flare stars up to hot supergiants, as well as in stellar chromospheres and coronae, in atmospheres of unstable and anomalous stars, in circumstellar clouds and gaseous shells born in nova and supernova explosions, in diffuse nebulae and the interstellar medium, in interacting binary systems, in galaxies with emission lines, in quasars, etc. The last thirty years have seen a turning-point in our knowledge concern ing the very nature of planetary nebulae (PNs). The radio emission of PNs was discovered after it was predicted theoretically. On the other hand, the powerful infrared emission discovered both in the continuum and in emission lines was never expected., Books<

2010, ISBN: 9783642082450

[ED: Softcover], [PU: Springer / Springer Berlin Heidelberg / Springer, Berlin], Planetary nebulae are the classic subject of astrophysics. The physical pro cesses occurring in this highl… Mehr…

[ED: Softcover], [PU: Springer / Springer Berlin Heidelberg / Springer, Berlin], Planetary nebulae are the classic subject of astrophysics. The physical pro cesses occurring in this highly ionized gaseous medium, the formation of emis sion lines in clearly specified conditions, the continuous emission extending from the far ultraviolet up to infrared and radio frequencies, the generation of exotic forms of radiation predicted by atomic physics, along with methods for deciphering the observed spectra and detecting physical and kinematic parameters of the radiating medium, etc. - all these problems form the solid foundations of the physical theory of gaseous nebulae. They are an essential part of the arsenal of powerful tools and concepts without which one cannot imagine understanding and interpreting the enormous diversity of processes taking place in the Universe - in gaseous envelopes surrounding the stars of various classes, from cool dwarfs and flare stars up to hot supergiants, as well as in stellar chromospheres and coronae, in atmospheres of unstable and anomalous stars, in circumstellar clouds and gaseous shells born in nova and supernova explosions, in diffuse nebulae and the interstellar medium, in interacting binary systems, in galaxies with emission lines, in quasars, etc. The last thirty years have seen a turning-point in our knowledge concern ing the very nature of planetary nebulae (PNs). The radio emission of PNs was discovered after it was predicted theoretically. On the other hand, the powerful infrared emission discovered both in the continuum and in emission lines was never expected. 2010. xv, 513 S. XV, 513 p. 235 mm Versandfertig in 6-10 Tagen, DE, [SC: 0.00], Neuware, gewerbliches Angebot, Offene Rechnung (Vorkasse vorbehalten)<

2005, ISBN: 9783642082450

[ED: Taschenbuch], [PU: Springer Berlin Heidelberg], Neuware - Planetary nebulae are the classic subject of astrophysics. The physical pro cesses occurring in this highly ionized gaseous … Mehr…

[ED: Taschenbuch], [PU: Springer Berlin Heidelberg], Neuware - Planetary nebulae are the classic subject of astrophysics. The physical pro cesses occurring in this highly ionized gaseous medium, the formation of emis sion lines in clearly specified conditions, the continuous emission extending from the far ultraviolet up to infrared and radio frequencies, the generation of exotic forms of radiation predicted by atomic physics, along with methods for deciphering the observed spectra and detecting physical and kinematic parameters of the radiating medium, etc. - all these problems form the solid foundations of the physical theory of gaseous nebulae. They are an essential part of the arsenal of powerful tools and concepts without which one cannot imagine understanding and interpreting the enormous diversity of processes taking place in the Universe - in gaseous envelopes surrounding the stars of various classes, from cool dwarfs and flare stars up to hot supergiants, as well as in stellar chromospheres and coronae, in atmospheres of unstable and anomalous stars, in circumstellar clouds and gaseous shells born in nova and supernova explosions, in diffuse nebulae and the interstellar medium, in interacting binary systems, in galaxies with emission lines, in quasars, etc. The last thirty years have seen a turning-point in our knowledge concern ing the very nature of planetary nebulae (PNs). The radio emission of PNs was discovered after it was predicted theoretically. On the other hand, the powerful infrared emission discovered both in the continuum and in emission lines was never expected., DE, [SC: 0.00], Neuware, gewerbliches Angebot, 235x155x29 mm, 536, [GW: 803g], Banküberweisung, PayPal, Klarna-Sofortüberweisung, Internationaler Versand<

2010, ISBN: 9783642082450

Springer Berlin Heidelberg, Taschenbuch, Auflage: Softcover reprint of hardcover 1st ed. 1997, 532 Seiten, Publiziert: 2010-02-19T00:00:01Z, Produktgruppe: Buch, Hersteller-Nr.: 180 black… Mehr…

Springer Berlin Heidelberg, Taschenbuch, Auflage: Softcover reprint of hardcover 1st ed. 1997, 532 Seiten, Publiziert: 2010-02-19T00:00:01Z, Produktgruppe: Buch, Hersteller-Nr.: 180 black & white illustrations, 93 blac, 1.63 kg, Geophysik, Geowissenschaften, Naturwissenschaft & Mathematik, Fachbücher, Kategorien, Bücher, Astronomie, Naturwissenschaften & Technik, Geologie, Ingenieurwissenschaft & Technik, Theoretische Physik, Astrophysik, Fremdsprachige Bücher, Featured Categories, Englische Bücher, 7c9a6c79-19ea-4dea-90da-d7d47042d341_2301, 7c9a6c79-19ea-4dea-90da-d7d47042d341_0, Arborist Merchandising Root, acc906d0-2585-4921-a56f-3ff277850936_4901, acc906d0-2585-4921-a56f-3ff277850936_0, Special Features Stores, Taschenbücher, acc906d0-2585-4921-a56f-3ff277850936_4201, Springer Berlin Heidelberg, 2010<

2010, ISBN: 9783642082450

Springer Berlin Heidelberg, Taschenbuch, Auflage: Softcover reprint of hardcover 1st ed. 1997, 532 Seiten, Publiziert: 2010-02-19T00:00:01Z, Produktgruppe: Buch, Hersteller-Nr.: 180 black… Mehr…

Springer Berlin Heidelberg, Taschenbuch, Auflage: Softcover reprint of hardcover 1st ed. 1997, 532 Seiten, Publiziert: 2010-02-19T00:00:01Z, Produktgruppe: Buch, Hersteller-Nr.: 180 black & white illustrations, 93 blac, 1.63 kg, Geophysik, Geowissenschaften, Naturwissenschaft & Mathematik, Fachbücher, Kategorien, Bücher, Astronomie, Naturwissenschaften & Technik, Geologie, Ingenieurwissenschaft & Technik, Theoretische Physik, Astrophysik, Fremdsprachige Bücher, Featured Categories, Englische Bücher, 7c9a6c79-19ea-4dea-90da-d7d47042d341_2301, 7c9a6c79-19ea-4dea-90da-d7d47042d341_0, Arborist Merchandising Root, acc906d0-2585-4921-a56f-3ff277850936_4901, acc906d0-2585-4921-a56f-3ff277850936_0, Special Features Stores, Taschenbücher, acc906d0-2585-4921-a56f-3ff277850936_4201, Springer Berlin Heidelberg, 2010<