activity
20112026
most citedOutflow dynamics of dust-driven wind models and implications for cool envelopes of PNe

7 citations · 16 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Molecular cloud dispersal traced by the ionized carbon 158 micron line

L. Bonne, N. Schneider, S. Dannhauer +14

Feedback from massive stars in the form of radiation and winds impacts the associated host molecular cloud. Feedback can disperse cloud material and lead to the destruction of the…

astro-ph.GA2025★ 3 cited

[C II]-deficit caused by self-absorption in an ionized carbon-filled bubble in RCW79

Eduard Keilmann, Simon Dannhauer, Slawa Kabanovic +12

Recent spectroscopic observations of the [C II] 158 fine-structure line of ionized carbon (C), using the Stratospheric Observatory for Infrared Astronomy (SOFIA)…

astro-ph.GA2025

Application of resolved low-J multi-CO line modeling with RADEX to constrain the molecular gas properties in the starburst M82

Valencia Zhang, Jakob den Brok, Qizhou Zhang +10

The distribution and physical conditions of molecular gas are closely linked to star formation and the subsequent evolution of galaxies. Emission from carbon monoxide (CO) and its…

astro-ph.SR2019★ 6 cited

Interferometric observations of SiO thermal emission in the inner wind of M-type AGB stars IK Tauri and IRC+10011

J. L. Verbena, V. Bujarrabal, J. Alcolea +2

Context. AGB stars go through a process of strong mass-loss that involves pulsations of the atmosphere, which extends to a region where the conditions are adequate for dust grains…

astro-ph.SR2011★ 7 cited

Outflow dynamics of dust-driven wind models and implications for cool envelopes of PNe

J. L. Verbena, K. -P. Schröder, A. Wachter

The density profiles of cool envelopes of young Planetary Nebulae (PNe) are reminiscent of the final AGB outflow history of the central star, so far as these have not yet been tran…