activity
20062022
most citedResolving the stellar activity of the Mira AB binary with ALMA

218 citations · 2.2k across the 58 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 160 cited

On the reliability of mass-loss-rate estimates for AGB stars

Sofia Ramstedt, Fredrik L. Schoeier, Hans Olofsson +1

In the recent literature there has been some doubt as to the reliability of CO multi-transitional line observations as a mass-loss-rate estimator for AGB stars. Mass-loss rates for…

astro-ph2008★ 99 cited

Circumstellar water vapour in M-type AGB stars: Radiative transfer models, abundances and predictions for HIFI

Matthias Maercker, Fredrik L. Schoeier, Hans Olofsson +2

Aims: By performing a detailed radiative transfer analysis, we determine fractional abundances of circumstellar H2O in the envelopes around six M-type asymptotic giant branch stars…

astro-ph2007★ 18 cited

Embedded Stellar Populations towards Young Massive Star Formation Regions I. G305.2+0.2

S. N. Longmore, M. Maercker, S. Ramstedt +1

We present deep, wide-field J, H and Ks images taken with IRIS2 on the Anglo Australian Telescope, towards the massive star formation region G305.2+0.2. Combined with 3.6, 4.5, 5.8…

astro-ph2007

The physics and chemistry of circumstellar envelopes of S-stars on the AGB

S. Ramstedt, F. L. Schoeier, H. Olofsson

The S-stars have been suggested to be a brief transitional phase as stars evolve from oxygen-rich M-type stars into carbon stars, through the dredge up of carbon from He-shell burn…

astro-ph2007★ 1 cited

Photospheric and chromospheric activity on EY Dra

H. Korhonen, K. Brogaard, K. Holhjem +4

Magnetic activity in the photosphere and chromosphere of the M dwarf EY Dra is studied and possible correlations between the two are investigated using photometric observations in…

astro-ph2006★ 55 cited

Mass-loss properties of S-stars on the AGB

S. Ramstedt, F. L. Schoeier, H. Olofsson +1

We have used a detailed non-LTE radiative transfer code to model new APEX CO(J=3-2) data, and existing CO radio line data, on a sample of 40 AGB S-stars. The derived mass-loss-rate…