Infrared knots along protostellar jets

DOI

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).

Cone search capability for table J/A+A/419/999/object (Jet positions (from Simbad))

Identifier
DOI http://doi.org/10.26093/cds/vizier.34190999
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/419/999
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/419/999
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/419/999
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/419/999
Provenance
Creator Giannini T.; McCoey C.; Caratti o Garatti A.; Nisini B.; Lorenzetti D.,Flower D.
Publisher CDS
Publication Year 2004
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; Interstellar medium; Natural Sciences; Physics; Stellar Astronomy