OH masers in W3(OH)

DOI

Recent studies of methanol and ground-state OH masers at very high spectral resolution have shed new light on small-scale maser processes. The nearby source W3(OH), which contains numerous bright masers in several different transitions, provides an excellent laboratory for high spectral resolution techniques. We present a model of W3(OH) based on European VLBI Network (EVN) observations of the rotationally excited 6030 and 6035MHz OH masers taken at 0.024km/s spectral resolution.

Cone search capability for table J/ApJ/668/331/table1 (Detected 6030 and 6035MHz masers in W3(OH))

Cone search capability for table J/ApJ/668/331/table2 (Zeeman pairs and associations)

Identifier
DOI http://doi.org/10.26093/cds/vizier.16680331
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/668/331
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/668/331
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/668/331
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/668/331
Provenance
Creator Fish V.L.; Sjouwerman L.O.
Publisher CDS
Publication Year 2010
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