• Produktbild: Planetary and Proto-Planetary Nebulae: From IRAS to ISO
  • Produktbild: Planetary and Proto-Planetary Nebulae: From IRAS to ISO
Band 135

Planetary and Proto-Planetary Nebulae: From IRAS to ISO Proceedings of the Frascati Workshop 1986, Vulcano Island, September 8–12, 1986

Fr. 72.90

inkl. gesetzl. MwSt., Versandkostenfrei


Beschreibung

Produktdetails

Einband

Taschenbuch

Erscheinungsdatum

26.09.2011

Herausgeber

Andrea Preite Martinez

Verlag

Springer Netherland

Seitenzahl

302

Maße (L/B/H)

25.4/17.8/1.7 cm

Gewicht

583 g

Auflage

Softcover reprint of the original 1st ed. 1987

Sprache

Englisch

ISBN

978-94-010-8228-0

Beschreibung

Produktdetails

Einband

Taschenbuch

Erscheinungsdatum

26.09.2011

Herausgeber

Andrea Preite Martinez

Verlag

Springer Netherland

Seitenzahl

302

Maße (L/B/H)

25.4/17.8/1.7 cm

Gewicht

583 g

Auflage

Softcover reprint of the original 1st ed. 1987

Sprache

Englisch

ISBN

978-94-010-8228-0

Herstelleradresse

Springer-Verlag KG
Sachsenplatz 4-6
1201 Wien
AT

Email: GPSR Kontakt

Noch keine Bewertungen vorhanden

Verfassen Sie die erste Bewertung zu diesem Artikel

Helfen Sie anderen Kundinnen und Kunden durch Ihre Meinung.

Kundinnen und Kunden meinen

Bewertungen (0)

  • Produktbild: Planetary and Proto-Planetary Nebulae: From IRAS to ISO
  • Produktbild: Planetary and Proto-Planetary Nebulae: From IRAS to ISO
  • Session I..- Infrared emission from young planetary nebulae.- Advances in knowledge of planetary nebulae from UV astronomy.- Status of the spectroscopic survey of planetary nebulae.- Session II..- Announcement — “The Strasbourg-ESO Catalogue of galactic planetary nebulae”.- IRAS Additional Observations of planetary nebulae.- Spectroscopy at 8–13pm as a probe of the carbon to oxygen ratio in planetary nebulae.- Session III..- Protoplanetary nebulae.- The evolution from Miras to planetary nebulae as derived from observations of Miras and OH/IR stars.- The position of PN nuclei in the H-R diagram: present status.- On the nitrogen and helium enrichment of the interstellar medium.- Temperatures, luminosities and mass loss rates for PN nuclei.- An outflow model for bipolar planetary nebulae and the case of NGC 6302.- Session IV..- Mass loss and the transition of an AGB star to a central star of a planetary nebula.- Observational constraints to the theory of planetary nebulae evolution.- Session V..- Rambling along a Schoenberner track: nebular evolution and NLTE stellar atmospheres.- Evolution of hot subdwarfs — an empirical approach.- Excitation of planetary nebulae and evolution of their central star.- Ionisation and dynamical structure of planetary nebulae.- Formation and structure of nebulae around symbiotic objects based on radio to x-rays observations (a review).- Session VI..- The peculiar planetary nebula NGC 2346 and its nucleus.- NGC 2346. Visible and IR observations of several mass-loss episodes?.- Infrared and optical spectroscopy of the suspected planetary nebula He 2–77.- Contribution of nebular emission lines to IRAS photometric survey fluxes.- Infrared characteristics of Polycyclic Aromatic Hydrocarbons and the interpretation of IR astronomical spectra.- Near-Infrared photometry of IRAS planetary nebulae.- The effect of line emission on the IRAS data of planetary nebulae.- Session VII..- Modeling the thermal emission from dust in planetary nebulae.- Evolution of dust in planetary nebulae.- Observations of the spectrum of the interplanetary dust emission.- Session VIII..- The Infrared Space Observatory (ISO) project.- Final Discussion..- Discussion introduced by: S.R.Pottasch.- V.Weidemann.- L.F.Rodríguez.- R.S.Clegg.- P.Harrington.- N.Panagia.- M.F.Kessler.- Index of Subjects.- Index of Astronomical Objects.