Rings and filaments: The remarkable detached CO shell of U Antliae

Franz Kerschbaum, Matthias Maercker, Magdalena Brunner, Marko Mecina, Claudia Paladini, M Lindqvist, H. Olofsson, Elvire De Beck, Martin A. T. Groenewegen, E. Lagadec, Shazrene Mohamed, Sofia Ramstedt, Wouter H. T. Vlemmings, Markus Wittkowski

Veröffentlichungen: Beitrag in FachzeitschriftArtikelPeer Reviewed

Abstract

Aims. Our goal is to characterize the intermediate age, detached shell carbon star U Antliae morphologically and physically in order to study the mass-loss evolution after a possible thermal pulse. Methods. High spatial resolution ALMA observations of unprecedented quality in thermal CO lines allow us to derive first critical spatial and temporal scales and constrain modeling efforts to estimate mass-loss rates for both the present day as well as the ejection period of the detached shell. Results. The detached shell is remarkably thin, overall spherically symmetric, and shows a barely resolved filamentary substructure possibly caused by instabilities in the interaction zone of winds with different outflow velocities. The expansion age of the detached shell is of the order of 2700 yr and its overall width indicates a high expansion-velocity and high mass-loss period of only a few hundred years at an average mass-loss rate of ≠10 -5 M · yr -1. The post-high-mass-loss-rate-epoch evolution of U Ant shows a significant decline to a substantially lower gas expansion velocity and a mass-loss rate amounting to 4 × 10 -8 M · yr -1, at present being consistent with evolutionary changes as predicted for the period between thermal pulses.

OriginalspracheEnglisch
AufsatznummerA116
Seitenumfang8
FachzeitschriftAstronomy & Astrophysics
Jahrgang605
DOIs
PublikationsstatusVeröffentlicht - Sep. 2017

ÖFOS 2012

  • 103003 Astronomie
  • 103004 Astrophysik

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