L1489IRS observed by the submillimeter array Virtual Observatory Resource

Authors

1. Brinch
2. C.
3. Crapsi
4. A.
5. Jorgensen
6. J.
7. K.
8. Hogerheijde
9. M.
10. R.
11. Hill
12. T.

Published by

CDS

Abstract

Submillimeter Array observations of the Young Stellar Object L1489IRS (IRAS 04016+2610). These include images of the continuum at 267 GHz (1.12 mm) and line emission of the HCO+ J=3-2 transition at 267.55762 GHz. The HCO+ image is available in two different (u,v)-weighting schemes, natural and uniform, optimizing for S/N and resolution respectively. The continuum image is only available in uniform weighting. The synthesized beam size is 1".

Keywords

1. young-stellar-objects
2. infrared-sources
3. millimeter-astronomy
4. submillimeter-astronomy
5. radio-astronomy

Bibliographic source Bibcode

2007A&A...475..915B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/475/915

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/475/915

Document Object Identifer DOI

doi:10.26093/cds/vizier.34750915

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/475/915
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/475/915
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/475/915

IVOA Table Access TAP

https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).