H2O maser emissions of IRAS 19134+2131

DOI

Using the Very Long Baseline Array at six epochs, we have observed H_2_O maser emission in the preplanetary nebula IRAS 19134+2131 (I19134), in which the H_2_O maser spectrum has two groups of emission features separated in radial velocity by ~100km/s. We also obtained optical images of I19134 with the Hubble Space Telescope to locate the bipolar reflection nebula in this source for the first time.

Cone search capability for table J/ApJ/669/424/table2 (Parameters of the detected H_2_O maser features)

Identifier
DOI http://doi.org/10.26093/cds/vizier.16690424
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/669/424
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/669/424
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/669/424
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/669/424
Provenance
Creator Imai H.; Sahai R.; Morris M.
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; Cosmology; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics