2010, ISBN: 9048157587

[EAN: 9789048157587], New book, [SC: 9.63], [PU: Springer Netherlands Dez 2010], PHOTOMETRY; PLANET; SMOOTHED-PARTICLEHYDRODYNAMICS(SPH); SPECTROSCOPY; STARS; STELLAREVOLUTION, This item … Meer...

[EAN: 9789048157587], New book, [SC: 9.63], [PU: Springer Netherlands Dez 2010], PHOTOMETRY; PLANET; SMOOTHED-PARTICLEHYDRODYNAMICS(SPH); SPECTROSCOPY; STARS; STELLAREVOLUTION, This item is printed on demand - it takes 3-4 days longer - Neuware -The term proto-planetary nebulae (PPNe) in the context of the late stages of stellar evolution was created only slightly more than 20 years ago to express the belief that in the near future these objects will become planetary nebulae (PNe). The first proto-planetary nebulae (called also post-Asymptotic Giant Branch, or shortly post-AGB objects) AFGL 2688 and AFGL 618 were discovered in mid seventies in course of the Air Force Sky Survey. Investigation of this phase of stellar evolution developed very rapidly in 1980's after the IRAS mission when it became clear that proto-planetary nebulae emit a significant part of their energy in the mid-and far-infrared. Hundreds of new candidates have been proposed but the recognition of the real proto-planetary nebulae is not a simple task and needs a substantial effort to exclude cases that represent different evolutionary stages. High resolution spectroscopy of stellar atmospheres is of much importance in this respect. Surprisingly, only a small group of central stars, the so called 21 11m emitters, show chemical signatures of the 3 rd dredge up process. Very recently, a more detailed studies of mid-infrared spectra from the Infrared Space Observatory (ISO) allow for a better understanding of chemical composition and evolution of circumstellar material around these stars. A new impetus in the field of proto-planetary nebulae research was started in the 1990's with high spatial resolution imaging in mid-infrared and optical wavelength ranges. 472 pp. Englisch, Books<

2010, ISBN: 9789048157587

[ED: Softcover], [PU: Springer / Springer Netherlands], The term proto-planetary nebulae (PPNe) in the context of the late stages of stellar evolution was created only slightly more than … Meer...

[ED: Softcover], [PU: Springer / Springer Netherlands], The term proto-planetary nebulae (PPNe) in the context of the late stages of stellar evolution was created only slightly more than 20 years ago to express the belief that in the near future these objects will become planetary nebulae (PNe). The first proto-planetary nebulae (called also post-Asymptotic Giant Branch, or shortly post-AGB objects) AFGL 2688 and AFGL 618 were discovered in mid seventies in course of the Air Force Sky Survey. Investigation of this phase of stellar evolution developed very rapidly in 1980's after the IRAS mission when it became clear that proto-planetary nebulae emit a significant part of their energy in the mid-and far-infrared. Hundreds of new candidates have been proposed but the recognition of the real proto-planetary nebulae is not a simple task and needs a substantial effort to exclude cases that represent different evolutionary stages. High resolution spectroscopy of stellar atmospheres is of much importance in this respect. Surprisingly, only asmall group of central stars, the so called 21 11m emitters, show chemical signatures of the 3 rd dredge up process. Very recently, a more detailed studies of mid-infrared spectra from the Infrared Space Observatory (ISO) allow for a better understanding of chemical composition and evolution of circumstellar material around these stars. A new impetus in the field of proto-planetary nebulae research was started in the 1990's with high spatial resolution imaging in mid-infrared and optical wavelength ranges. 2010. xxi, 448 S. XXI, 448 p. 240 mm Versandfertig in 6-10 Tagen, DE, [SC: 0.00], Neuware, gewerbliches Angebot, Offene Rechnung (Vorkasse vorbehalten)<

2010, ISBN: 9048157587

[EAN: 9789048157587], New book, [SC: 12.25], [PU: Springer Netherlands], PHOTOMETRY; PLANET; SMOOTHED-PARTICLEHYDRODYNAMICS(SPH); SPECTROSCOPY; STARS; STELLAREVOLUTION, Druck auf Anfrage … Meer...

[EAN: 9789048157587], New book, [SC: 12.25], [PU: Springer Netherlands], PHOTOMETRY; PLANET; SMOOTHED-PARTICLEHYDRODYNAMICS(SPH); SPECTROSCOPY; STARS; STELLAREVOLUTION, Druck auf Anfrage Neuware - Printed after ordering - The term proto-planetary nebulae (PPNe) in the context of the late stages of stellar evolution was created only slightly more than 20 years ago to express the belief that in the near future these objects will become planetary nebulae (PNe). The first proto-planetary nebulae (called also post-Asymptotic Giant Branch, or shortly post-AGB objects) AFGL 2688 and AFGL 618 were discovered in mid seventies in course of the Air Force Sky Survey. Investigation of this phase of stellar evolution developed very rapidly in 1980's after the IRAS mission when it became clear that proto-planetary nebulae emit a significant part of their energy in the mid-and far-infrared. Hundreds of new candidates have been proposed but the recognition of the real proto-planetary nebulae is not a simple task and needs a substantial effort to exclude cases that represent different evolutionary stages. High resolution spectroscopy of stellar atmospheres is of much importance in this respect. Surprisingly, only a small group of central stars, the so called 21 11m emitters, show chemical signatures of the 3 rd dredge up process. Very recently, a more detailed studies of mid-infrared spectra from the Infrared Space Observatory (ISO) allow for a better understanding of chemical composition and evolution of circumstellar material around these stars. A new impetus in the field of proto-planetary nebulae research was started in the 1990's with high spatial resolution imaging in mid-infrared and optical wavelength ranges., Books<

2009, ISBN: 9789048157587

Series Editor: Gorny, S. K. Springer Netherlands, Taschenbuch, Auflage: Softcover reprint of hardcover 1st ed. 2001, 472 Seiten, Publiziert: 2009-12-28T00:00:01Z, Produktgruppe: Buch, Her… Meer...

Series Editor: Gorny, S. K. Springer Netherlands, Taschenbuch, Auflage: Softcover reprint of hardcover 1st ed. 2001, 472 Seiten, Publiziert: 2009-12-28T00:00:01Z, Produktgruppe: Buch, Hersteller-Nr.: 9789048157587, 0.66 kg, Medizin, Kategorien, Bücher, Astronomie, Naturwissenschaften & 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, Szczerba, R. Springer Netherlands, 2009<

2009, ISBN: 9789048157587

Series Editor: Gorny, S. K. Springer Netherlands, Taschenbuch, Auflage: Softcover reprint of hardcover 1st ed. 2001, 472 Seiten, Publiziert: 2009-12-28T00:00:01Z, Produktgruppe: Buch, Her… Meer...

Series Editor: Gorny, S. K. Springer Netherlands, Taschenbuch, Auflage: Softcover reprint of hardcover 1st ed. 2001, 472 Seiten, Publiziert: 2009-12-28T00:00:01Z, Produktgruppe: Buch, Hersteller-Nr.: 9789048157587, 0.66 kg, Medizin, Kategorien, Bücher, Astronomie, Naturwissenschaften & 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, Szczerba, R. Springer Netherlands, 2009<