NGC 2071 water masers

DOI

We have mapped the water maser emission associated with the infrared centers IRS 1 and IRS 3 of the NGC 2071 IR star-forming region at four epochs over ~4 months with the Very Long Baseline Array. We detected 269 maser features with ~1km/s line widths and measured 30 proper motions. In each infrared center, the water maser emission appears to trace parts of a protostellar disk and collimated outflow.

Identifier
DOI http://doi.org/10.26093/cds/vizier.15810325
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/581/325
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/581/325
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/581/325
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/581/325
Provenance
Creator Seth A.C.; Greenhill L.J.; Holder B.P.
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