TWINKLING STARS The disappearing SiO masers of W Aql
Paper i proceeding, 2012

W Aql is a binary S-type AGB star showing SiO maser emission. The dust distribution around the star is asymmetric, possibly indicating gravitational interaction between the binary pair. There are indications that the gas distribution also exhibits asymmetries. To investigate the source of the circumstellar structures, we applied for and were rewarded VLBI time to map the distribution of the SiO masers around this source and to constrain the presence and distribution of a possible magnetic field. Using VERA observations we also aim at measuring an accurate parallax to determine the binary separation, however, from showing peak emission of 21 Jy in June 2010, the SiO(1-0) v=1 line at 43 GHz has now disappeared. We find no correlation with the stellar pulsational period.

stars: AGB and post-AGB

masers

stars: mass loss

Författare

S. Ramstedt

Argelander-Institut für Astronomie

Wouter Vlemmings

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

S. Mohamed

South African Astronomical Observatory

Y.K. Choi

Max-Planck-Gesellschaft

Hans Olofsson

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

Proceedings of the International Astronomical Union

1743-9213 (ISSN) 1743-9221 (eISSN)

Vol. 8 5287 260-261

The XXVIIIth General Assembly of the International Astronomical Union (IAU)
Beijing, China,

Ämneskategorier

Astronomi, astrofysik och kosmologi

Fundament

Grundläggande vetenskaper

Infrastruktur

Onsala rymdobservatorium

DOI

10.1017/S1743921312007107

Mer information

Senast uppdaterat

2021-02-18