Chemical tracers of a highly eccentric AGB–main-sequence star binary
Artikel i vetenskaplig tidskrift, 2024

Binary interactions have been proposed to explain a variety of circumstellar structures seen around evolved stars, including asymptotic giant branch (AGB) stars and planetary nebulae. Studies resolving the circumstellar envelopes of AGB stars have revealed spirals, disks and bipolar outflows, with shaping attributed to interactions with a companion. Here we use a combined chemical and dynamical analysis to reveal a highly eccentric and long-period orbit for W Aquilae, a binary system containing an AGB star and a main-sequence companion. Our results are based on anisotropic SiN emission, the detections of irregular NS and SiC emission towards the S-type star, and density structures observed in the CO emission. These features are all interpreted as having formed during periastron interactions. Our astrochemistry-based method can yield stringent constraints on the orbital parameters of long-period binaries containing AGB stars, and will be applicable to other systems.

Författare

Taissa Danilovich

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Monash University

KU Leuven

J. Malfait

KU Leuven

M. Van De Sande

University of Leeds

M. Montargès

Observatoire de Paris

P. Kervella

Observatoire de Paris

F. De Ceuster

KU Leuven

A. Coenegrachts

KU Leuven

T. J. Millar

Queen's University Belfast

A. M.S. Richards

University of Manchester

L. Decin

KU Leuven

University of Leeds

C. A. Gottlieb

Harvard-Smithsonian Center for Astrophysics

C. Pinte

Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)

Monash University

Elvire De Beck

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

D. J. Price

Monash University

K. T. Wong

Institut de Radioastronomie Millimétrique (IRAM)

Uppsala universitet

J. Bolte

Christian-Albrechts-Universität zu Kiel

KU Leuven

K. M. Menten

Max-Planck-Gesellschaft

A. Baudry

Laboratoire d'Astrophysique de Bordeaux

A. de Koter

KU Leuven

Anton Pannekoek Institute for Astronomy

S. Etoka

University of Manchester

D. Gobrecht

Göteborgs universitet

M. Gray

University of Manchester

National Astronomical Research Institute of Thailand

F. Herpin

Laboratoire d'Astrophysique de Bordeaux

M. Jeste

Max-Planck-Gesellschaft

E. Lagadec

Laboratoire Joseph-Louis Lagrange

S. Maes

KU Leuven

I. McDonald

University of Manchester

Open University

L. Marinho

Laboratoire d'Astrophysique de Bordeaux

H. S.P. Müller

Universität zu Köln

B. Pimpanuwat

University of Manchester

National Astronomical Research Institute of Thailand

J. M.C. Plane

University of Leeds

R. Sahai

California Institute of Technology (Caltech)

Sofia Wallström

KU Leuven

J. Yates

University College London (UCL)

A. Zijlstra

University of Manchester

Nature Astronomy

23973366 (eISSN)

Vol. 8 3 308-327

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1038/s41550-023-02154-y

Mer information

Senast uppdaterat

2024-03-30