SiO maser survey in Galactic center

We have surveyed ~400 known large-amplitude variables within 15' of the galactic center in the SiO J=1-0 v=1 and 2 maser lines at 43GHz, resulting in 180 detections. SiO lines were detected from 16 other sources located within 20" of the program objects. The detection rate of 48% is comparable to that in bulge IRAS surveys.

Cone search capability for table J/PASJ/56/261/table2 (SiO detections)

Cone search capability for table J/PASJ/56/261/table3 (Negative results)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/PASJ/56/261
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASJ/56/261
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASJ/56/261
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/PASJ/56/261
Provenance
Creator Deguchi S.; Imai H.; Fujii T.; Glass S.; Ita Y.; Izumiura H.; Kameya O.,Miyazaki A.; Nakada Y.; Nakashima J.
Publisher CDS
Publication Year 2006
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; Cosmology; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics