Infrared knots along protostellar jets Virtual Observatory Resource

Authors

1. Giannini T.
2. McCoey C.
3. Caratti o Garatti A.
4. Nisini B.
5. Lorenzetti D.,Flower D.

Published by

CDS

Abstract

We present the near infrared spectra (0.9-2.5 micron) of protostellar jets (HH 24-26, HH72, BHR71). The observations were carried out with Sofi at R~600 with the 1x290arcsec slit. The spectra are dominated by H2 rovibrational lines (v up 5). Faint emission from ionized material in form of [FeII] and [SII] lines is also recognizable. The tables contain the observed lines together with the measured flux. The reported error derives from the rms of the baseline, multiplied by the width of the instrumental profile (30 Angstrom).

Keywords

1. interstellar-medium
2. infrared-sources
3. molecular-clouds
4. young-stellar-objects

Bibliographic source Bibcode

2004A&A...419..999G

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/419/999

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/419/999

Document Object Identifer DOI

doi:10.26093/cds/vizier.34190999

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/419/999
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/419/999
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/419/999

IVOA Table Access TAP

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IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
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http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/419/999/object?