Infrared knots along protostellar jets (Giannini+, 2004)

Details Infrared knots along protostellar jets (Giannini+, 2004) Infrared knots along protostellar jets (Giannini+, 2004)

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34190999g&link_type=abstract

VizieR On-line Data Catalog: J/A+A/419/999. Originally published in: 2004A&A...419..999G

Physics

Interstellar Medium, Infrared Sources, Molecular Clouds, Ysos

Scientific paper

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).
(4 data files).

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