Spectroscopy of H_2_ towards HH91A Virtual Observatory Resource

Authors

1. Gredel R.

Published by

CDS

Abstract

Optical and near-infrared spectroscopy of molecular hydrogen in interstellar shocks provide a very powerful probe of the physical conditions that prevail in interstellar shocks. Integral-field spectroscopy of H_2_ in the optical wavelength region and complementary long-slit near-infrared spectroscopy towards HH91A are used to characterize the ro-vibrational population distribution among H_2_ levels with excitation energies up to 30000cm^-1^.

Keywords

1. young-stellar-objects
2. spectroscopy

Bibliographic source Bibcode

2007A&A...474..941G

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/474/941

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/474/941

Document Object Identifer DOI

doi:10.26093/cds/vizier.34740941

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/474/941
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/474/941
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/474/941

IVOA Table Access TAP

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