SiO maser emission in evolved stars

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.36420213
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/642/A213
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/642/A213
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/642/A213
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/642/A213
Provenance
Creator Gomez-Garrido M.; Bujarrabal V.; Alcolea J.; Soria-Ruiz R.; de Vicente P.; Desmurs J.-F.
Publisher CDS
Publication Year 2020
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy