activity
20192026
most citedDistance estimates for AGB stars from parallax measurements

81 citations · 113 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

Periodic activity on the (sub)mm surface of the AGB star Mira A

M. Andriantsaralaza, B. Bojnordi Arbab, W. Vlemmings +7

Evolved stars on the asymptotic giant branch (AGB) lose mass through stellar winds launched from their dynamic extended atmospheres. Recent high-angular-resolution observations of…

astro-ph.SR2026

A giant magnetic eruption from the asymptotic giant branch star Mira A

W. Vlemmings, M. Andriantsaralaza, B. Bojnordi Arbab +14

Mass loss during the advanced evolutionary stages of low- and intermediate-mass stars is traditionally attributed to dust-driven winds, whereas the influence of magnetic fields rem…

astro-ph.SR2026

Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars. III. SiO and SiS abundances

R. Unnikrishnan, E. De Beck, L. -Å. Nyman +9

The present understanding of C-rich AGB chemistry largely relies on observations of the archetypal carbon star IRC+10216. Current molecular abundance estimates for carbon stars are…

astro-ph.SR2025★ 1 cited

Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars. II. Abundances and spatial distributions of CS

R. Unnikrishnan, M. Andriantsaralaza, E. De Beck +9

The circumstellar envelopes (CSEs) of asymptotic giant branch (AGB) stars harbour a rich variety of molecules and are sites of complex chemistry. Our current understanding of the c…

astro-ph.SR2022★ 81 cited

Distance estimates for AGB stars from parallax measurements

M. Andriantsaralaza, S. Ramstedt, W. H. T Vlemmings +1

Estimating the distances to asymptotic giant branch (AGB) stars using optical measurements of their parallaxes is not straightforward because of the large uncertainties introduced…

astro-ph.SR2021★ 12 cited

DEATHSTAR: Nearby AGB stars with the Atacama Compact Array II. CO envelope sizes and asymmetries: The S-type stars

M. Andriantsaralaza, S. Ramstedt, W. H. T. Vlemmings +13

We aim to constrain the sizes of the CO circumstellar envelopes (CSEs) of 16 S-type stars, along with an additional 7 and 4 CSEs of C-type and M-type AGB stars, respectively. We ma…