SiO maser emission in evolved stars Virtual Observatory Resource

Authors

1. Gomez-Garrido M.
2. Bujarrabal V.
3. Alcolea J.
4. Soria-Ruiz R.
5. de Vicente P.,Desmurs J.-F.

Published by

CDS

Abstract

We aim to study the time evolution of the SiO maser lines in Mira-type and semi-regular variables at short timescales. We observed the SiO maser lines at 7mm and 3mm using the 40m Yebes antenna and the 30m IRAM telescope, respectively, with a minimum spacing of 1 day. We studied the semi-regular variables RX Boo and RT Vir and the Mira-type variables U Her, R LMi, R Leo, and chi Cyg.

Keywords

1. Variable stars
2. Giant stars
3. Astrophysical masers
4. Radio astronomy
5. Spectroscopy

Bibliographic source Bibcode

2020A&A...642A.213G

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/642/A213

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/642/A213

Document Object Identifer DOI

doi:10.26093/cds/vizier.36420213

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/642/A213
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/642/A213
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/642/A213

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).