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Table · dataset · 2020

SiO maser emission in evolved stars

Listed in IVOA Registry (Virtual Observatory)

We aim to study the time evolution of the SiO maser lines in Mira-type and semi-regular variables at short timescales.

Description

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.

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Stated by source
Radio
Inferred from text
Astronomical sciences 72%
Provenance · 1 source records, 9 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/642/a21315 d agoJSON v1
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concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (72%)
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