collaborators

15 papers

astro-ph200883 cited

Multiple ring nebulae around blue supergiants

S. M. Chita, N. Langer, A. J. van Marle +2

In the course of the life of a massive star, wind-wind interaction can give rise to the formation of circumstellar nebulae which are both predicted and observed in the nature. We p…

astro-ph200842 cited

Jets as diagnostics of the circumstellar medium and the explosion energetics of supernovae: the case of Cas A

K. M. Schure, J. Vink, G. García Segura +1

We present hydrodynamical models for the Cassiopeia A (Cas A) supernova remnant and its observed jet / counter-jet system. We include the evolution of the progenitor's circumstella…

astro-ph200824 cited

The planetary nebula NGC 1360, a test case of magnetic collimation and evolution after the fast wind

M. T. Garcia-Diaz, J. A. López, G. Garcia-Segura +2

The central star of this nebula has an observed intense magnetic field and the fast wind is no longer present, indicating that a back flow process has probably developed. Long-slit…

astro-ph200743 cited

The circumstellar medium around a rapidly rotating, chemically homogeneously evolving, possible gamma-ray burst progenitor

Allard Jan van Marle, Norbert Langer, Sung-Chul Yoon +1

Rapidly rotating, chemically homogeneously evolving massive stars are considered to be progenitors of long gamma-ray bursts. We present numerical simulations of the evolution of th…

astro-ph200742 cited

Constraints on gamma-ray burst and supernova progenitors through circumstellar absorption lines. (II): Post-LBV Wolf-Rayet stars

A. J. van Marle, N. Langer, G. garcia-Segura

Van Marle et al. (2005) showed that circumstellar absorption lines in early Type Ib/c supernova and gamma-ray burst afterglow spectra may reveal the progenitor evolution of the exp…

astro-ph200642 cited

The Dynamical Evolution of Planetary Nebulae After the Fast Wind

G. Garcia-Segura, J. A. Lopez, W. Steffen +2

In this paper we explore the dynamics of ionization bounded planetary nebulae after the termination of the fast stellar wind. When the stellar wind becomes negligible, the hot, sho…