activity
19982014
most citedA hydrodynamical study of multiple-shell planetary nebulae. III. Expansion properties and internal kinematics: Theory versus observation

44 citations · 88 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2014★ 44 cited

A hydrodynamical study of multiple-shell planetary nebulae. III. Expansion properties and internal kinematics: Theory versus observation

D. Schoenberner, R. Jacob, H. Lehmann +5

We present the result of a study on the expansion properties and internal kinematics of round/elliptical planetary nebulae of the Milky Way disk, the halo, and of the globular clus…

astro-ph2006

New observations of the halo radial temperature structure in NGC7662

C. Sandin, D. Schoenberner, M. M. Roth +4

We report on our studies of the physical structure of the planetary nebula (PN) NGC7662. Using (3D) Integral Field Spectroscopy we have been able to measure the electron temperatur…

astro-ph2006★ 43 cited

Stellar archaeology: the evolving spectrum of FG Sge

C. S. Jeffery, D. Schoenberner

Over an interval of 120 years, the extraordinary object FG Sge has been transformed from a hot post-AGB star to a very luminous cool supergiant. Theoretically, this evolution has b…

astro-ph2000★ 1 cited

The evolution of helium white dwarfs: III. On the ages of millisecond pulsar systems

D. Schoenberner, T. Driebe, T. Bloecker

We employed recently computed evolutionary white-dwarf models with helium cores, supplemented by heavier models with carbon-oxygen cores, in order to investigate the ages of millis…

astro-ph1999

On the Transition from AGB Stars to Planetaries: The Spherical Case

Detlef Schoenberner, Matthias Steffen

We discuss the basic physical model and the relevant processes responsible for creating and shaping planetary nebulae out of a cool AGB wind envelope. We show that a hydrodynamical…

astro-ph1998

Evolutionary Models of White Dwarfs with Helium Cores

T. Driebe, D. Schoenberner, T. Bloecker +1

We present seven evolutionary tracks for low-mass white dwarfs with helium cores, ranging in mass from 0.179 to 0.414 Msol. We generated the pre-white dwarf models from a 1 Msol se…